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POLITECNICO DI MILANO
DIPARTIMENTO DI FISICA
PhD course in Physics
XXV cycle
DEVELOPMENT AND APPLICATION OF A RAMAN
MAPPING INSTRUMENT FOR THE STUDY OF
CULTURAL HERITAGE
Supervisor: Prof. Gianluca Valentini
Tutor: Prof. Rinaldo Cubeddu
PhD coordinator: Prof. Paola Taroni
Candidate: BRAMBILLA ALEX
2010 - 2012
2
“In all things of nature there is something of the marvelous”
Aristotle
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4
Summary.
Summary. 4
Abstract. 7
Introduction. 10
CHAPTER I
RAMAN SPECTROSCOPY. 13
I.1 Molecular vibrations. 13
Vibrational energy. 14
Normal modes of vibration. 15
I.2 Classical theory of Raman scattering. 19
Susceptibility and polarizability. 20
Rayleigh and Raman scattering. 21
I.3 Quantum theory of Raman scattering. 24
Time dependent perturbations: the second order transition probability. 25
A semi-classical expression for Raman effect. 28
Full quantum approach. 32
Second quantization. 33
The Kramers-Heisenberg formula. 36
General considerations. 39
I.4 The cross section. 41
I.5 Surface Enhanced Raman Scattering. 43
Bibliography. 45
CHAPTER II
THE REMOTE RAMAN SCANNER. 47
II.1. Raman spectroscopy in Cultural Heritage. 47
II.2. The aim of the project. 49
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Raman imaging. 50
Remote Raman sensing. 51
Portable Raman instruments. 53
II.4. Remote Raman Scanner: the layout. 55
II.5. RRS: the standard components 57
Semiconductor laser. 57
Galvanometric mirrors. 59
Holographic notch filter. 60
Czerny-Turner spectrograph. 60
Charge coupled device (CCD). 61
Optical fibers. 62
II.6 RRS: the custom-made systems. 63
The optical system. 63
The software. 67
Bibliography. 71
CHAPTER III.
RRS AT WORK: TESTS AND CASE STUDIES. 77
III.1 Characterization of the performances. 77
Assessment of the depth of the field of view. 78
Assessment of the field of view. 79
Assessment of the spectral accuracy. 80
Assessment of the spatial resolution. 80
III.2 A multi-analytical approach to a model painting. 82
Reflectance spectra and reconstructed maps. 83
XRF analysis. 87
Flexible Raman mapping. 91
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III.3 Identification of white and fluorescent pigments. 94
III.4 Analysis of samples from the “Memoriale italiano” of Auschwitz. 97
III.5 Study of a 3D plastic object 100
III.6. Mapping of a rock sample. 102
Bibliography. 106
CHAPTER IV
SERS ANALYSIS OF AMINO ACIDS WITH A PORTABLE INSTRUMENT.
108
IV.1. The aim of the work. 108
IV.2 SERS of amino acids. 109
IV.3 SERS with metal nanoparticles. 112
IV.4 The portable instrument. 115
IV.5 Tests and results. 116
Raman spectra of amino acids. 117
Analysis of liquid samples. 120
Analysis of dried solutions. 122
Dependence of L-Met spectra on pH. 124
Distinguishing two amino acids. 125
Towards a more complex sample. 128
IV.5 Perspectives. 129
Bibliography. 135
CHAPTER V
CONCLUSION. 140
Acknowledgements. 144
7
Abstract.
Raman spectroscopy is a consolidated technique for the analysis of materials: it is
based on the identification of the frequency shifts undergone by light scattered by a
molecule; this behavior is due to an interaction of the incident photons with the
vibrational quanta of the involved material. The possibility to obtain information on
a molecular scale about the chemical identity of a sample in a non-destructive way,
makes this method one of the favourite for the analysis of valuable objects, as it is in
case of Cultural Heritage. In this field of application it is particularly urgent the
necessity to monitor wide surfaces of heterogeneous objects often with an irregular
shape. Compared to a laboratory measurement, moreover, an in situ analysis implies
further requirements due to the dimensions and the portability of the employed
instrumentation, which must guarantee an adequate sensitivity to Raman signal
while keeping the necessarily limit of a non-invasive procedure.
To answer to these needs, a portable Raman spectroscopy system which works with
a non contact approach, has been conceived, designed and assembled. The device is
able to analyze a surface 5 cm wide placed at a distance of 20 cm with a flexible
mapping approach: a pair of galvanometric mirrors allows the deflection of the laser
beam, which is focused on the point of interest by a dedicated optical system. This
element was tailored to collect and guide the light scattered by the sample towards
the instruments of analysis (spectrograph and charged coupled device) which, like
the laser source, are remotely positioned and connected by optical fibers. This
solutions permits to keep the measuring probe light and small, and to mount it on a
tripod in order to ensure maximum flexibility and stability at the same time; the
instruments of analysis can be, alternatively, connected to a more conventional
Raman microscope when a deeper punctual analysis is needed. The chance of
performing remote measurements not only considerably widens the range of object
to study, but it also makes the device less affected by the vibrations which perturb
contact analysis when performed out of the laboratory environment; moreover, the
particular combination of the chosen optic elements ensures a depth of field ideal
for the analysis of three-dimensional objects.
8
The thesis treats the theoretical foundations of Raman spectroscopy to highlight its
potentialities and stress the common problematiques (in primis the low efficiency
with respect to competitive phenomena such as fluorescence); then, the phases of
the project of the Remote Raman device are reported together with the methods to
test its performances and features. One chapter is dedicated to the results of
punctual analysis and to the study of wide areas in samples of artistic or cultural
interest; whenever it is possible, these are compared to the information obtained by
other non-invasive techniques on the same objects. Last, surface-enhanced Raman
measurements on amino acids in low concentrations are reported as a preliminary
study for the analysis of organic traces in archaeological remains.
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10
Introduction.
The application of scientific techniques to the study of Cultural heritage is wide
reaching. Not only research groups of chemists, physicists, geologists, engineers and
biologists are growingly demanded to provide diagnostic methods for several kinds
of artefacts, but museums and conservation centers now rely on scientific pools of
specialists equipped with cutting-edge analytical tools. The information furnished by
analytical methods, yielding data on the atomic and the molecular composition
through spectroscopic techniques, for example, is valuable not only for historical or
scientific interest, but also important as data can support critical evaluation, the
authentication of a masterpiece, or guide the restoration operation.
Despite the fact that the role of scientific methods in humanistic studies such as
preservation, conservation and promotion of cultural heritage is now undisputed,
the research of new methods of application continues to develop. The typical issues
related to the analysis of cultural heritage, which generally concern the need to
interact in the softest possible way with the object of interest, represent a
continuous challenge for researchers, who look for techniques capable of providing
significant information with a non-destructive or, preferably, a non-invasive
approach. These two requirements have lead to the spread of optical analytical
techniques, like reflectance spectroscopy, Infrared absorption spectroscopy and
Raman spectroscopy, for the characterization of surfaces of works of art; in most of
their applications, these methods rely on a laser as a light source, therefore they
benefit from the explosion in development and expansion of these instruments in
the last decades. The parallel improvement and the declining price of light detectors,
in addition, has led to the birth of imaging versions for optical analyses: the
possibility of studying a large set of points on a surface with a single acquisition
further promotes the application of these techniques to the study of artworks.
Within this framework, this thesis presents a novel instrument for Raman
spectroscopy, able to perform a stand-off mapping of a macroscopic surface at a safe
working distance of approximately 20 cm and thus particularly suitable for
analyzing valuable objects. Commercially available Raman Spectrometers which are
marketed for the analysis of works of art work either in contact or at very short
working distances (on the order of millimeters). The aim of the reported work has
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been to build an instrumental apparatus ready to be operated in the laboratory as
well as on site; the need for a significant flexibility in the measurement of different
points of a representative area, led to the design and development of a dynamic
mapping device, which can selectively illuminate and stimulate the Raman
scattering of each point within its field of view, without any relative movement
between the probe head and the target object. The layout of the set-up has been
oriented towards a remote instrument, capable of being employed even in
uncomfortable environments thanks to a portable probe head and to a working
distance of 20 cm, sufficient to ensure a non-invasive approach to the object of
interest, and at the same time to reduce the sensitivity to vibrations.
A thorough study of Raman scattering has been the first, indispensible step in the
design of the measurement apparatus. In Chapter 1, a description of the Raman
effect, as explained by the classic and the quantum theory, is presented, based on
some of the most common approaches followed in physics and chemistry. Particular
mention to the standard Raman event and to the enhancement to the effect provided
by the interaction with a metal substrate is made; one of the aims of the thesis,
indeed, is to determine how the adoption of suitable procedures and the
optimization of technological parameters can help the detection of the intrinsic
weak Raman scattering with a portable apparatus, whose acquisition is generally
more critical of bench-top instrument. In Chapter 2 the state of the art of Raman
mobile and stand-off devices is addressed; this study compares the proposed set-up
with available Raman mapping and imaging devices. In addition the choices
determined during the design and construction of the system are reviewed. With
Chapter 3, the performances of the completed set-up are reported: in this case, the
focus is on the capability of providing the identification of different kinds of
materials and samples of heterogeneous objects. The integration of the Raman
mapping instrument with other non-destructive analytical methods is evaluated on
a model of a painted panel, as the ultimate test of the application. In Chapter 4 tests
performed with a commercial mobile Raman instrument, chosen for a different kind
of analysis are reported: the study of organic fragments contained in ancient vessels
and pottery. For this specific purpose, research was carried out with a device with a
portable probe head but based on the traditional microscope layout. The novelty of
the chosen approach resides in the adoption of metal nanoparticles as a substrate to
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enhance the Raman cross section of the analytes, in this case simulated by solutions
of amino acids. The exploited technique, which goes under the name of Surface-
Enhanced Raman Spectroscopy (SERS), has been applied for the first time with a
portable Raman instrument on this kind of materials: amino acids and a small
peptide, in small concentrations have been chosen for the preliminary tests to assess
the detection limits for these organic materials. The reported results are the first
step towards the determination of a routine method that could be easily applied in
situ to reveal traces of biological materials on archaeological finds.
13
CHAPTER I
RAMAN SPECTROSCOPY.
Raman spectroscopy is based on the homonym effect, postulated by Smekal in 1923
[I.1] and first observed experimentally in 1928 by C.V. Raman and Krishnan [I.2]: in
the original experiment, for which Raman was awarded the Nobel prize in physics
two years later, sunlight was focused by a telescope onto a sample which was either
a purified liquid or a dust-free vapor. A second lens was placed by the sample to
collect the scattered radiation and a system of optical filters was used to show the
existence of scattered radiation with an altered frequency from the incident light –
the basic characteristic of Raman spectroscopy [I.3]. Inelastic scattering is due to the
interaction of the electromagnetic radiation with the level structure of a molecule or
a solid: the scattering event corresponds to a virtual transition (in a sense that will
be specified later) between rotational, vibrational or electronic levels triggered by
light and mediated by quanta of electromagnetic energy called photons. Commonly,
Raman spectroscopy is focused on the second type of these processes, involving
vibrational transitions. Together with infrared absorption, this technique is used to
obtain information about the structure and properties of molecules and solids in a
non destructive way [I.4].
I.1 Molecular vibrations.
A molecule is classically described as the collection of M nuclei and N electrons [I.5]
arranged in a stable configuration: if the positions of the nuclei are considered fixed,
each molecule can be associated to a “molecular point group”, which is a symmetry
group corresponding to a fixed point, the center of mass of the molecule. In the same
way, a crystal is described as the periodic distribution of a unit cell, made out of a set
of atoms, along each point of a spatial lattice, called Bravais lattice, generated by
14
three linearly independent vectors. Each crystal is associated to a crystallographic
group according to the symmetry of the point group of its cell, and to the symmetry
of the lattice [I.6]. The symmetry properties of molecules and solids are determinant
for the vibrational transitions which are observed with Raman, and in general
vibrational spectroscopy; this is true also in a negative sense, as it is for amorphous
materials, in which regularities are mostly absent and a statistical description of the
structure is necessary.
For the present discussion, the molecule is considered as the model for the classical
and quantum systems on which the Raman effect is treated: this allows the
treatment to be relatively compact and still valid for gaseous, liquid and many solid
samples; whenever it is needed, reference to crystals and amorphous materials will
be explicitly made.
Vibrational energy.
A common approximation when describing the molecule is to consider that the
motion of the electrons can be separated by the motion of nuclei. This assumption
(called Born-Oppenheimer approximation) is realistic, considering the ratio of the
masses of the electron and a generic nucleus: the motion of the electrons is faster
than the one of nuclei at least by 3 orders of magnitude, and so the latter are almost
“at rest” with respect to these particles. Thanks to Born-Oppenheimer
approximation, the problem to determine the dynamic of the electrons is solved
while maintaining fixed the positions of the nuclei (which appear in the solution as
parameters) and the electronic contribution obtained by this calculation is used to
describe the total energy of the system [I.5]. This separation of the electronic motion
and the nuclear motions is only an approximation which may break down in certain
cases, especially for high electronic states. If there were no interaction between the
two types of motions, there would be no Raman effect of any importance. However,
the coupling is small for the lowest electronic state [I.7].
The molecule, seen as a rigid body, can translate along three arbitrary Cartesian
axes: therefore, three of its 3M degrees of freedom represent its translations in
space. If the center of mass is then fixed, the molecule has 3M – 3 remaining degrees
of freedom: rotations around the coordinate axes represent three (or two, for a
linear molecule) of these degrees of freedom. Six (five) parameters are needed, thus,
15
to describe the molecule as a whole: the remaining 3M – 6 (or 3M – 5) degrees of
freedom describe, instead, the variations among the “standard” location of the nuclei
around the center of mass, i.e. the deformations of the molecule: these are called
vibrational degrees of freedom. The global energy of the isolated molecule can be
accordingly divided into four terms:
Emol = Eelectronic + Etranslational + Erotational + Evibrational (1.1)
From a quantum-mechanical point of view, each of this term is associated to a
component of the total molecular Hamiltonian.
ℋmol = ℋelectronic + ℋtranslational + ℋrotational + ℋvibrational (1.2)
Within the chosen approximation, the four terms are considered independent and so
the separation of variables within the Schrödinger’s equation for the molecule is
carried on, leading to a factorial expression for the wave function
Ψmol = Ψelectronic Ψtranslational Ψrotational Ψvibrational (1.3)
The reported considerations refer to a molecule in absence of an external potential:
further considerations are necessary to take into account the interaction of this
system with light, as it will become clearer in the following sections.
Normal modes of vibration.
The translational motion of the molecule does not ordinarily give rise to radiation.
Classically, this happens because acceleration of charges is required for radiation.
The rotational motion causes practically observable radiation if, and only if, the
molecule has an electric (dipole) moment. The vibrational motions of the atoms
within the molecule may also be associated with radiation if these motions alter the
electric moment [I.7].
Vibrations, as we have seen, correspond to any displacement among the positions of
the atoms which do not alter the position of the center of mass nor its angular
momentum. The dynamic description of these vibrations must consider, therefore,
forces internal to the molecule: at a first approximate analysis, the intra-molecular
potential can be limited to the nearest neighbor atoms. This is equivalent to consider
the intra-molecular potential V(R) of a biatomic molecule, which is, if referred to the
equilibrium distance R0 between the two atoms, clearly asymmetric (fig.I.1); the
16
energy of the molecule tends to infinite if the atoms are too close, and instead
reaches a saturation for very long distances, when it is equal to the work necessary
to dissociate the molecule. Even though, in the range in which the molecule is stable
(below the dissociation value), it is possible to approximate the potential with a
harmonic oscillator. The expression of the intra-molecular potential can indeed be
expanded around its minimum, and it is convenient before performing this
operation, to introduce a suitable frame of reference.
Fig.I.1. The intra-molecular potential curve V(R) for a bi-atomic molecule (blue curve). Without any
loss of generality, in the graph the dissociation energy value is set equal to 0. The green curve refers
to the harmonic approximation.
To start with, a standard Cartesian system of coordinates xi is chosen. A molecule
constituted by M atoms is described by a set of 3M coordinates, so i runs from 1 to
3M; at the equilibrium configuration, these respectively assume the values ci. The
displacement along each coordinate, therefore, will be calculated as the difference
Δxi = xi – ci; clearly, the time derivatives (indicated by a dot over the letter) of the
initial Cartesian coordinates are exactly equal to the corresponding time derivative
17
of the displacement coordinates. A set of the so-called mass-weighted coordinates qi
is constructed according to the relationship
q m
where, obviously, the mis are equal in groups of three in a row because they refer to
the same atom. This choice permits to simplify the kinetic energy expression
q
The series expansion of the potential energy is, accordingly, carried out in powers of
qi:
q
q
q q
q q
,
A comfortable choice of V0 is to set it to zero, without any loss of generality. The
second term in the right-hand side of the equation is automatically zero for the
definition of the equilibrium position (the derivative is evaluated for qi = 0). If the
expansion is arrested at the second order, therefore, only the last term is surviving,
and it can be synthetically written as
q q
q q
,
f q q
where the second order derivatives of V, evaluated in the equilibrium position, can
be considered as the elements fij of a 3M × 3M dynamic matrix F. The equations of
motion of the molecule are described by the solutions of the 3M Lagrange equations
d
dt
q
q
which, with the chosen approximation, can be written as a set of 3M simultaneous
second-order linear differential equations, each one closely resembling the well-
known equations of the harmonic oscillator:
q f q
(1.4)
(1.5)
(1.6)
(1.7)
(1.8)
(1.9)
18
If a tentative solution of the form
q cos t
where Ai, and are properly chosen constants, is substituted, the set of differential
equations is transformed in a set of 3M simultaneous algebraic equations in Ai
f
Where the ij symbol stands for the Kronecker delta. The solutions of these
equations are not trivial only for a special set of s (which have the physical
dimensions of pulsations): clearly, this is but a secular equation for the dynamic
matrix F. For each particular value of , namely k, a certain set of amplitude Ai,
namely Aik, is obtained; however, it can be shown that only the ratios between the
different Ais is determined per each k. Therefore, the choice of convenience, if there
is no strict constraint given by the initial conditions on qi, is to set the values for
which the modulus of the vector [A1k, A2k, 3Mk] is unitary. These normalized
vectors are indicated as aik, and they can be grouped in a matrix called A.
It can be demonstrated, as well, that six out of the 3M eigenvalues of the matrix F are
zero: the null roots of the secular equation correspond to null pulsations, which
means that six degrees of freedom, as previously reported, are not ascribable as
vibrations. This means that, through a proper choice of the coordinates, this can be
reduced to a 3M – 6 square matrix without any loss of information. It can be easily
shown that this transformation is performed by multiplying the qi vector by the
matrix A of the normalized eigenvectors. Since there are only 3M – 6 eigenvectors,
each one made of 3M elements, the transformation produces naturally a new system
of 3M – 6 coordinates Qk, called vibrational coordinates. On the basis of the
vibrational coordinates, the dynamic matrix is diagonal, i.e. the harmonic oscillators
are decoupled.
This rather laborious analysis of the intra-molecular potential has the advantage to
introduce all the necessary elements to thoroughly describe molecular vibrations.
From the initial truncation of the series expansion, called Mechanic Harmonic
approximation, it was possible to derive the dynamic matrix F. The eigenvalues k of
this matrix correspond to the pulsations of the oscillations of the atoms around their
(1.10)
(1.11)
19
equilibrium positions, their amplitude along the coordinate axis (except for a
multiplicative factor) given by the eigenvectors Aik. The equations (1.10) therefore,
describe motions in which all the atoms vibrate with a single frequency ωk = k½ in
phase: these are called vibrational modes of the molecule, and are described by the
vibrational coordinates Qk as independent harmonic oscillators.
Qk = Qk0 cos (ωkt + k) (1.12)
For the properties here described, the modes are orthogonal and normal: this
property allows the decomposition of any collective displacement of the nuclei of the
molecule in a series built over a basis of independent oscillations. In addition, it is
worth to anticipate that the decomposition along the normal modes of vibration is
necessary for the quantum description of Raman effect, because only within this
frame of reference the vibrational eigenfunction Ψvibrational can be written as the
product of independent quantum oscillators.
It is possible to calculate the force constants of each harmonic oscillator starting
from ab initio Hartree-Fock or density functional theory (DFT) methods: the
symmetry of the potential function will allow the reduction in size of the dynamic
matrix to a group of smaller matrices, one for each irreducible representation of the
molecular point group. Each normal mode of a molecule forms a basis for an
irreducible representation of the point group of the molecule itself [I.8]. Group
theory can be used to recover the normal mode coordinates starting from the
geometry of the molecule: the use of the so-called character table permits not only to
list the vibrational modes, but it also assigns them to the respective class of the
symmetry operations that build up the point group [I.8]. At the same time, the study
of the molecule symmetry allows the identification of degenerate vibration
frequencies and it is crucial for the determination of a mode’s activity in the Infrared
or Raman spectrum.
I.2 Classical theory of Raman scattering.
Raman effect is classically explained in terms of the dependence of the polarizability
of the molecule on the normal modes of vibration of the molecule. The scattering of
an electromagnetic wave, indeed, can be expressed in terms of the polarization
20
induced in the material by the incoming electric field (the role of the magnetic field
can be neglected for the present treatment). It is known, in fact, that an oscillating
dipole absorbs end emits energy in the form of electromagnetic waves. Polarization,
indicated by the letter P, is a vector which describes the average (and hence,
macroscopic) contribution of the electric dipoles p which can be associated to the
molecules constituting the material. There are two possible models to describe this
quantity: one introduces the concept of susceptibility and is more suitable for
describing the behavior of a solid, being it an isolator or a metal; whereas for
molecules it is convenient to introduce the polarizability. Both these descriptions
consider only the linear dependence in the electric field E, but a more thorough
theory of scattering must include higher order terms1 as well (which are necessarily
taken into account for an explanation of phenomena such as hyper Raman or
stimulated Raman scattering, not considered here).
Susceptibility and polarizability.
The first approach follows a global description of the scattering material.
Polarization, then, can be written as the difference between the dielectric
displacement vector, D and the field in the vacuum multiplied by the permittivity of
the vacuum ε0. Polarization can be expressed, as well, making explicit the
proportionality to the electric field: the constant which relates the vector P and E is,
apart from a factor of ε0, known as susceptibility and written as χ
P = D - ε0E ε0 εR -1) E ε0 χ E (1.13)
χ is dependent only on the properties of the materials and on the frequency of the
electric field; in the most general case, where P is not necessarily parallel to E, it is a
tensor.
If the description of the electric induction is measured on the single molecule, it is
convenient to express the polarization in terms of the induced dipole momentum p;
1 The total time-dependent induced electric dipole moment vector of a molecule may be written as the sum of a series of time-dependent vectors as follows: p = p
(1) + p
(2) + p
(3) + …
where p(1)
= αE, p(2)
= ½ βEE, p(3)
= ⅙ γEEE …[I.12] and the order of magnitude of the addends
p(n) decreases dramatically with the order n.
21
this is related to the electric field through the polarizability α, which is again a tensor
(p can be non parallel to E).
p = α E (1.14)
where α is measured in C m2/V unity and its components are indicated with the
notation αρσ, the indices ρ and σ assume the values x, y, z. Except in very special
circumstances, the Raman polarizability tensor is real and symmetric, i.e. αρσ = ασρ;
it is always possible, moreover, to make it diagonal by a proper choice of the
coordinate frame of reference.
If corrections for the so-called local field are negligible, it is possible to correlate the
two expressions 1.1 and 1.2 through the definition of polarization P as the average
dipole momentum multiplied by the number of molecules per unit of volume.
P = <p> N/V (1.15)
Only in particularly simplified cases, however (for example, a gas in standard
conditions of temperature and pressure [I.9]), it is possible to trace an easy
relationship between susceptibility and the polarizability tensor,
χ = αN/ ε0V (1.16)
where α is the scalar corresponding to the average of the elements αii of the
polarizability matrix in its diagonal form [I.10]. More generally, it can be said that
the electric susceptibility is the sum of the polarizabilities of the single molecules
contained in the unit volume, divided per the dielectric constant and the volume
itself.
Rayleigh and Raman scattering.
For the present description it is sufficient to refer to the induced dipole moment of
the molecule, and therefore, to the polarizability. This quantity is dependent on the
distribution of the electrons around the ions of the molecule; the perturbation
introduced by the incident electric field produces a displacement of the charge
distributions with respect to their position at the equilibrium: this phenomenon can
be expressed by the concept of an induced dipole. Polarizability depends also on the
characteristics of the exciting field: the response of the charge distribution is not
instantaneous [I.11], so the effect of applying a constant perturbation is not the same
22
of an electric field which varies with a pulsation ω. In synthesis, from a
phenomenological viewpoint, it is possible to state that polarizability is a function of
the angular frequency of the electric field
p(ω) = α(ω)E(ω) (1.17)
for the simplest description of the elastic (or Rayleigh) scattering, that is of the
scattering of light at the same frequency of the exciting electromagnetic wave. The
actual form of this tensor can be derived by a series of descriptions, one of which is
represented by the Lorentz model of the atom as a harmonic oscillator with a
natural pulsation ω0.
More generally, the induced dipole possesses a spectral distribution which is not
simply a Dirac delta centered on the angular frequency of the exciting electric field.
This fact implies that the polarizability not only is a function of this variable, but it is
also relevantly influenced by the natural pulsations ωk of the vibrations of the
molecule. The induced dipole emitting at a generic angular frequency ωS, where S
stands for Scattering, can be described by the equation
p(ωS) = α(ω, ωk)E(ω) (1.18)
given vibration will hence induce a “modulation” of the linear optical polarizability
with a frequency equal to that of the internal vibration. Each of this motions can be
decomposed, as we have seen, in a basis of orthonormal vibrational coordinates Qk.
It is possible to expand in a Taylor series every matrix element of α according to the
normal coordinates of vibration Qk of the molecule and neglecting, for clarity of the
notation, the dependence on the pulsation of the exciting field. The expansion of the
polarizability component αij, where the indices i and j can vary among the chosen
reference axes, is
αij = αij,0 ∑k αij/ Qn)0 Qk + ½ ∑k,k’ 2αij/ Qk Qk’)QkQk’ (1.19),
stopping after the second order; the subscript 0 indicates that the derivatives are
evaluated at the origin of the frame of reference of the vibrational coordinates. The
electric harmonic approximation consists in arresting the expansion at the first
order, and here this approach is chosen. Since the expansion in power series is valid
for all components of the polarizability, equation 1.18 can be rewritten in vector
23
form. If the perturbing electric field is a monochromatic plane wave of equation E =
E0 cos(ω0t), we obtain
p = αk,0E0 cos(ωt ∑k α/ Qk)0 Q0E0 cos(ωkt + k) cos(ω0t) =
= αk,0E0 cos(ωt ½ ∑k α/ Qk)0 Q0E0 cos((ω ± ωk)t + k)
Where the quantity α/ Qk)0 is called derived polarizability tensor or Raman
tensor of the normal mode k. It is apparent how, besides the presence of the so-
called Rayleigh component at ω, the emergence of two symmetric terms ω – ωk
(Stokes) and ω + ωk (anti-Stokes) per each vibrational mode is justified simply by
trigonometry [I.12]. The classical expression for Raman effect, therefore, is related
to the polarizability components which have a non-zero derivative with respect to a
molecular vibration at the equilibrium position of the molecule. The main
consequence of this fact is that not all vibrational modes can be investigated by the
detection of Raman scattering, but vibrations which correspond to a zero value for
the Raman tensor are said to be Raman-inactive.
The classical interpretation of Rayleigh and Raman scattering can, in conclusion, be
summarized as follows. If the molecule is at rest, the induced moment, and therefore
the scattered light, has the same frequency as the incident light. If, however, the
molecule is rotating or vibrating, this is not necessarily the case, because the
amplitude of the induced electric moment may depend on the orientation of the
molecule and the relative positions of its atoms. Since the configuration changes
periodically because of rotation and vibration, the scattered radiation is
''modulated" by the rotational and vibrational frequencies so that it consists of light
of frequencies equal to the sum and to the difference of the incident frequency and
the frequencies of the molecular motions, in addition to the incident frequency [I.7].
Another difference is that Rayleigh scattering happens always in phase with the
incident radiation, whereas Raman scattering bears an arbitrary phase relation due
to the phase k of the involved molecular vibrations [I.12].
(1.20)
24
Fig. I.2. Example of dependence of the polarizability from the vibrational modes and correspondent
Raman activity for a linear molecule of the type A-B-A (for example, CO2)[I.12]
I.3 Quantum theory of Raman scattering.
It has been shown that a classical theory of Raman scattering is possible, even if it
adopts a phenomenological viewpoint. Nonetheless, some of the conclusions which
can be drawn, for example, from equation 1.20 can be misleading. For instance,
correlating the Raman intensity (proportional to the square of the scattered field) to
the Raman tensor would predict equal intensities for the inelastic and superelastic
component of the spectrum, since the magnitude of the derivative of the
polarizability is the same for both the branches: prediction that is strongly denied by
the actual spectroscopic measurements, in which Stokes scattering is most easily
detected. Moreover, dependence of Raman on the vibrations of the molecule would
infer that no Raman spectrum can be obtained by molecules on the vibrational
ground state, contrarily to what is observed. This deficiency of the classical
treatment, in particular, is to be related to the absence of the zero-point energy in a
harmonic oscillator problem, which leads to the impossibility to describe
phenomena like spontaneous emission of light. A quantum treatment of the
25
scattering process is, therefore, necessary, even for a treatment that does not
include nonlinear phenomena such as hyper Raman scattering.
From a quantum viewpoint, Raman scattering may be treated as the inelastic
collision of an incident photon ħωo with a molecule on the initial energy level Enm
[I. 3]. Following the collision, a photon ħωs with different energy is detected and the
molecule is found on another energy level En. The energy difference ΔE = En-Em =
ħωnm, when positive, may appear as vibrational, rotational of electronic energy of
the molecule: this variation is called Stokes shift. If the molecule is initially in a
excited state, the difference can be negative and the superelastic photon scattering is
indicated as an anti-Stokes event. If the character of a vibration to be or not Raman
active can in principle be derived by classical or semi-classical description, the
intensity of a Raman band is not easily predicted by these treatments. For this
reason, a more correct formula for the Raman cross section of a vibration must be
the aim of the full quantum theory of light scattering.
Time dependent perturbations: the second order transition
probability.
In a quantum system described by the time independent Hamiltonian ℋ0, every
eigenstate is described by the symbol |u⟩ and corresponds to an eigenfucntion Ψu
and to an eigenvalue Eu: this eigenvalue governs the exponential time dependence of
the eigenfunction
Ψ ⟩ ⟩ e
/
Since the probability that the quantum system is in a state n is equal to the square
modulus of |Ψn⟩, it does not change with time: therefore, the description of any
transitions between two states must take into account the time dependence.
In Schrödinger’s representation the operators are constant whereas the wave
functions evolve with time. If a perturbation ℋi = ℋi(t) is introduced, so that ℋi(t)
Ŵ t > , the states u⟩ (from now on |u⟩), are still an orthonormal base for the
vector space. This means that a generic state |Ψ(t)⟩ can be expressed as
Ψ t ⟩ au t e i ut/ u⟩
u
(1.21)
(1.22)
26
provided that the complex coefficients au are functions of the time. As for the time-
independent case, their square modulus is proportional to the probability to find the
system in a state |n⟩ at the time t. If the initial state of the system is the state |m⟩, the
summation at time t = 0 is degenerate. Thanks to this property, an expression for an
can be obtained by substitution of 1.1 into the Schrödinger equation; this, after a
simple multiplication by ⟨n| eiEnt/ of both sides leads to
an
t
i au t e
– i u – n t/
u
n W u
Exact solution for this set of equations is possible only for limited cases (for
example, a two-level system). In general, it is necessary to proceed by successive
approximations by developing each coefficient au as a sum of different order terms.
au = au(0) + au(1) + au(2)
this approach is known as perturbative method. The validity of this method is
confirmed, in the case here discussed, as long as the applied electric field is a small
perturbation from the typical electric fields felt by electrons and atoms in molecules
(which is of the order of 1010 V/m)[ I.11]. A Raman scattering description must
consider at least to stop this expansion to the second order, because from a particle
viewpoint this phenomenon involves two photons. Since the perturbation is small,
the first order solution for a generic final state f is obtained by neglecting all terms
with u ≠ m in the equation . 3 they are strictly null at t , thus reducing the
summation to a single element
an
t
i e – i m – n t/ n W m
and integrating with time τ (with the consideration that the perturbing Hamiltonian
matrix has zero diagonal elements, i.e ⟨u Ŵ u⟩ = 0).
an
i e – i m – t/
τ
n W m dt
For higher orders, the procedure is iterative: the second order solution is given by
substituting into 1.2.2 the first order expression of the an. The resulting expression is
(1.24)
(1.25)
(1.26)
(1.23)
27
a
i a
t
e – – /
n W u dt
in which the expression of the first order solution can be made explicit. This
equation is valid for each choice of interacting Hamiltonian, provided that the
perturbation is “turned on” at time t . The electromagnetic field incident on the
molecule can be represented as a periodic potential e pressed by the function Ŵ t
Ŵ+ e–iωt Ŵ- eiωt, with Ŵ+ = Ŵ-† to make sure it is Hermitian and, hence, physically
meaningful. Spatial dependence of the electromagnetic field is thought as negligible
along the more significant dimension of the considered system, as it is for a molecule
exposed to NIR or visible light. If the energy difference between the state |n⟩ and |m⟩
is written as ħωmn, the expression for the first order coefficient is
a
n W m
e –
ω – ω n W m
e
ω ω
which is able to describe optical transitions where a single photon is involved
(absorption). The second order coefficient, substituting 1.28 into 1.27 and exploiting
the exponential dependence of the perturbing Hamiltonian with time, can be
synthetically written as
a
i
n W u u W m
ω ω
e
e dt
This expression can be separated in the sum of six summations: according to the
presence of one or the opposite sign, it is possible to distinguish different domains
for the energy values of the involved eigenstates. The sign of Ŵ is plus if n > Em,
minus vice versa, whereas the sign between the angular frequencies is chosen
according to the position of the intermediate energy level |u⟩: in particular, it is +
when Eu > Em. The transition probability Pmn is evaluated as the square modulus of
the coefficient an, which according to eq. 1.24 is given by the sum of the two
components an(1) and an(2),
Pmn ≈ an(1) + an(2) |2
This is the complete probability that a transition between the levels m and n,
mediated by an electromagnetic field represented by the perturbing Hamiltonian Ŵ,
occurs: all phenomena which involve one or two photons interacting with the
system (atom or molecule) are therefore included. Despite its generality, it is
(1.29)
(1.30)
(1.27)
(1.28)
28
already possible to highlight some peculiarities in the formula above reported. First
of all, the presence of differences at the denominators hints at the possibility of
indefinitely high value (in practice limited by the uncertainty at which the energy of
the quantum states can be measured) for the probability transitions: in other words,
the expression takes into account the resonant behavior which characterizes the
interaction of an electric field whose frequency is correspondent to a “jump”
between two states in the quantum system considered. Additionally, the transition
probability is shown to be dependent on the off-diagonal matrix elements of the
perturbing Hamiltonian Ŵ, which can be written as an integral quantity:
W u W v W d
This matrix expression reveals how the introduced perturbation determines which
transition between the unperturbed set of quantum states is or not allowed. A
theory of Raman scattering must start from a meaningful expression of the
interaction of the exciting light with the molecule or solid and then consider all the
terms inside 1.30 corresponding to inelastic (or superelastic) scattering, i.e. where
the angular frequency of the incident electric field is shifted.
A semi-classical expression for Raman effect.
This description treats the interaction of a quantum system (the molecule), whose
Hamiltonian H0 can be expressed as in equation 1.3, with a classical electromagnetic
field: the energy contribution of this interaction is represented by the symbol ℋi.
The interaction Hamiltonian for a multiparticle system exposed to an
electromagnetic field does not show an easy to handle expression, so it is often
necessary to approximate it with the so-called Electric-Dipole (ED) Hamiltonian:
ℋi = ℋED = – E p
which is by far the most important contribution to the perturbing Hamiltonian; the
other terms (magnetic dipole, electric quadrupole etc.) arising from the interaction
are negligible as far as ℋED is not zero, so in most cases the approximation is
(1.32)
(1.31)
29
excellent2. The electric field E is supposed to be a plane monochromatic wave of
angular frequency ω, whereas the operator p is defined as the sum of all the
coordinate vectors of the nuclei and electrons,
where q is equal to ±e if a proton or an electron charge is considered. For Raman
scattering of molecule this definition works also in a simpler depiction, with rj being
the atoms coordinates and q the effective charges they carry on. Sometimes,
moreover, the total dipole moment of the molecule can be considered as the sum of
biatomic dipole contributions [I.12] constituted by the couple of nearest neighbor
atoms. The vector components of p, px, py, pz are similarly defined with respect to the
projection of rj and r along the Cartesian coordinates.
The following treatment is a synthesis of the approach followed by Placzek [I.14]: his
description of the Raman scattering does not explicitly proceed through the
transition probability expression, but an analogous method is used to determine the
form of the electric polarizability. A transition dipole, equivalent to the matrix
element of the dipole operator among the time dependent wave functions Ψ’n, Ψ’n of
the perturbed system, is introduced
(p)mn = ⟨Ψ’n| p |Ψ’m⟩
This transition dipole can be considered as the quantum equivalent of the
oscillating electric dipole of the classic description. Thanks to perturbation theory,
an expression of the transition dipole in terms of the non-perturbed eigenstates |u⟩
can be recovered. By arresting the expansion of the perturbed functions to the first-
order, and after grouping all the terms with the same frequency dependence, the
expression of the real component of the component ρ of the vector p, with the choice
of the symbol ωmn = (En – Em)/ , results3:
2 For linear processes in E such as standard Raman scattering it is sufficient to consider the electric dipole term: for a standard molecular transition, the electric quadrupole and magnetic dipole terms, which follow in the expansion of ℋi, are of the order of the so-called fine structure constant α ≈ 1/137 [2]. 3 A more rigorous expression takes into account the decay time of each intermediate state |u⟩, which, differently from the initial and final ones, does not need to be stationary. Considering these decays as constants removes the divergence caused by the difference at the denominators.
(1.33)
(1.34)
30
p
n p u u p m
ω ω e
n p u u p m
ω ω
e
∑
e
e c. c.
where c.c. stands for complex conjugate; the expression, rather cumbersome,
manages to express the transition dipoles in terms of the matrix element of the
dipole operator, evaluated on the unperturbed states; the terms can be grossly
divided in two, the ones oscillating at the frequency sum and the ones at the
difference. The latter take into account the three kinds of scattering, provided that
the quantity ω – ωnm is positive: Rayleigh is obtained for |m⟩ = |n⟩; the terms with
the frequency (ω + ωnm) at the exponential, instead, do not correspond to any
scattering process. Recalling the classical expression which relates the induced
dipole to the electric field, it is possible to derive an equation defining the so-called
general transition polarizability (α)fi, whose components are of the form
α
n p u u p m
ω ω
n p u u p m
ω ω
Fig. I.3. Pictorial representation of the vibrational transitions corresponding to the three kinds of
scattering. For the anti-stokes transition the order of the n and m states is reversed with respect to
the notation adopted here.
(1.36)
(1.35)
31
In principle, the calculus of polarizability, and hence of the Raman scattering cross
section, is made possible only through an accurate estimation of every energy level,
wave function and lifetime of the molecule. Fortunately, a series of general
assumptions can be made to apply this formula to concrete cases of studies. If the
energy of the incident photon, for example, is not sufficient to excite the molecule in
its first electronic level, and the ground electronic state is not degenerate, the
eigenstates involved in the matrix elements can be identified with the set of the
vibrational eigenfunctions (vi). The transition polarizability, therefore, can be
written in the compact form
α v α v
Other simplifications stand in less favorable cases, introducing the coupling between
electronic and nuclear motion can be as a second perturbation. In any case, it is
possible in the end to come to a more manageable formula of this sort, for the
scattered intensity summed over all the space directions:
This form, much like the Raman tensor of the classic description, allows a rapid
determination of the so-called selection rules which determine if a vibrational
transition can be triggered by Raman scattering. In the mechanical and electric
approximation, the transitions between pure vibrational states are possible if, and
only if, the variation of the quantum number is ±1. A more general formulation of
this constraint regards the symmetry representations of the elements involved in
the equation of the transition polarizability. These components transform as the
binary products x2, y2, z2, xy, xz and yz. Group theory characters tables, therefore,
show which irreducible representation correspond to Raman or IR active mode
according to the presence of these functions.
Γ1⊂Γ(vm)Γ(αρσ)Γ(vn)
Where Γ1 is the totally symmetric representation [I.8, I.12]. This general rule makes
no statement as to the intensity with which a permitted transition will appear in the
(1.37)
(1.38)
(1.39)
32
Raman spectrum; in a mono-dimensional case it can be described as an argument
based on the parity of the functions which concur to the product inside the integral
(1.37).
Full quantum approach.
The full quantum approach becomes necessary whenever a resonance phenomenon
is affecting the Raman scattering [I.15]: it is through this formulation, indeed, that
the role of the coupling between the photons and the electronic states of the
material can be evaluated.
In a multi-level atom or molecule, several processes can occur in presence of an
incoming electromagnetic radiation (fig. I.4). In terms of the quantum theory of light,
Raman scattering consists in the destruction of an incoming photon (of frequency ν,
pulsation ω = 2πν and wave vector k, k= w n(ω)/c) in correspondence with the
creation of a photon of a difference pulsation ωs and wave vector ks: the process
leaves the quantum system on a different energy level and can be considered
instantaneous [I.16]. It is, as well, a coherent event [I.4], in the sense that the two
phases must satisfy conservation of energy and momentum: the differences ω – ωs, k
– ks, are therefore associated with a transfer of energy and momentum to the
molecule. This transfer results, in the second case, in the excitation of one or more
vibrational modes; if the scattering material is a crystal, the Raman scattering
corresponds to the excitation of a so-called phonon, i.e. a quantized oscillation
distributed along the whole lattice. The key difference between Raman scattering
and fluorescence is that in Raman scattering the incident photon is not fully
absorbed and instead perturbs the molecule exciting or de-exciting vibrational or
rotational energy states. Contrastingly, in fluorescence the photon is completely
absorbed causing the molecule to jump to a higher electronic state, and then the
emitted photon is due to the molecule’s decay back to a lower energy state [I. 7].
Three terms contribute to the transition rate associated with this event (creation
followed by destruction, destruction followed by creation, creation and destruction
simultaneously occurring) according to the quantum mechanical description: in this
formalism there is no difference between the order in which the two events occur,
provided that the energy conservation is satisfied by their combination [I.16]. Each
of these terms, indeed, is multiplied by a Dirac delta along the ωs function centered
33
at ω – ωmn, where ωmn is the pulsation of the final state. However, as already
emphasized, the energy ω does not necessarily correspond to any electronic
transition energy and the photon of energy ωmn is not absorbed in the strict
spectroscopic sense, as there is no conservation of energy in this stage of the
process. The role of the incident radiation is rather to perturb the molecule and
open the possibility of spectroscopic transitions other than direct absorption. If ω
approaches an electronic transition energy, enhancement of the scattered intensity
is observed [I.12]. It is important to note that Raman scattering is not the absorption
of the photon, followed by the emission of a photon of less energy, that instead
describes fluorescence.
Fig.I.4. A comparison between the most important different transitions involving the interaction of a molecule
with photons in the visible-near infrared range, on a schematic energy diagram [I.23].
Second quantization.
A step further in the quantum theory of scattering needs the introduction of proper
quantum operator for electric field. Let us consider for the moment only one mode
of oscillation. Electromagnetic radiation with a single frequency ωk and a wave
vector k is fully described by the potential vector Ak(t) = Ak e-i(ωt-kr) + Ak* ei(ωt-kr). It is
34
associated with an energy term which can be suitably expressed as the energy of a
classical harmonic oscillator if quantities
are introduced. The expression for the energy is, therefore,
2ε0AkAk*V = ½ (pk2 + qk2ω2). (1.41)
The quantum solution for this kind of problems requires the replacement of the
classical quantities with suitable operators qk q , pk
p , which can be considered as
a coordinate and its momentum, since the commutation relationship gives [p k,q k] =
– i . The Schrödinger equation for this kind of potential gives as a solution a set of
discrete eigenvalues for the radiation energy En,k = ωk (nk + ½), where nk is an
integer. For this reason, it is possible to consider each contribute of ωk as a
quantum of energy, called photon; in this way, to each eigenvalue for energy a wave
function called “number state” or Fock state and corresponding to the presence of n
photons can be found. This number states are eigenfunctions not only of the
Hamiltonian, but of the number operator n k = âk †âk, given by the product of the so
called operators “creation” and “destruction” whose definition is respectively
These two operators are not observables, but they correspond to the addition and
subtraction of one quantum of energy to the eigenstates of the Hamiltonian,
provided that a minimum amount of energy ( ωk/2, zero-point energy) is
conserved, transforming them from |nk⟩ to |nk+1⟩ and |nk-1⟩ respectively.
The set of all the possible modes of the electromagnetic field in a cavity (or in free
space) can be regarded as the cumulative wave function of all the number states.
|{nk}⟩ = |nk1⟩|nk2⟩
(1.40)
(1.40b)
(1.42)
(1.42b)
(1.43)
35
There is always an infinite number of oscillators, so the |{nk}⟩ form a complete set of
state for the electromagnetic field in the cavity.
Starting from these functions it is possible to recover the expression for the
Potential vector with straightforward substitutions, and hence the quantum
expression for electric and magnetic field. Equations 1.44 and 1.44b give the
expression for the k mode of both fields.
These expressions are used when the perturbation is added to the Hamiltonian of
the molecule. If the interaction between the incoming electromagnetic wave and the
molecule is limited to ℋED, then the dipole momentum gives rise to the transition
dipole pfi,
To make explicit the transition nature of this quantity, the dipole is associated to the
transition operator |i⟩⟨j|, which, when applied to |j⟩ gives |i⟩ and gives zero with all
the other eigenstates. Thanks to the closure theorem, the expression of the dipole
operator p can be rewritten in a more significant form.
The explicit form of the quantum operator p in ℋED is, then
⟩ ⟨ ⟩ ⟨ ⟩⟨
,
and therefore the perturbing Hamiltonian can be written as
ℋ
,
⟩
⟨
This e pression is responsible of the transitions between the states j and I, with I ≠ j
since the terms with I = j are null because of integral of odd functions. From the
(1.44)
(1.44b)
(1.45)
(1.46)
(1.47)
36
matrix elements it is possible to calculate absorption and emission rates for a
generic atom and photon distributions.
Before moving to the application of this formula to the study of the interaction of
particles with electromagnetic field, it is convenient to remind that the harmonic
oscillator problem is actually a common approximation for many physical problems.
The same vibrational energy contribution within the global molecular Hamiltonian,
as it was shown, can be expanded up to the second order and hence, each vibrational
degree of freedom Qk possesses an energy
Ev,k = (vk + ½) ωk, vk , , ,
where k, running from 1 to 3M-6, is the index of the vibrational modes and not a
wave vector. Vibrations, therefore, are ruled by the same quantum operators
introduced for photons, applied to the normal modes Qk: q k, q k†for the destruction
and the creation of a vibrational quantum respectively. Equivalently to quanta of
electromagnetic energy, quanta of vibrations can be treated as particles, which
statistically behave as bosons.
The Kramers-Heisenberg formula.
In principle, the forces between the atoms can be calculated a priori from the
electronic wave equation, but in practice this is not mathematically feasible (except
for H2), and it is necessary to postulate the forces in such a manner as to obtain
agreement with experiments. Therefore, although it is theoretically possible to start
with a model consisting of electrons and nuclei interacting by a Coulomb potential
and obeying the laws of quantum mechanics, in practice it is necessary to assume
the nature of the equilibrium configuration and of the forces between the atoms, so
that it seems more desirable to start with the model in which the atoms are the units
[20]. This system is then exposed to the perturbation of the electromagnetic field, in
the form of the quantum operators obtained by the second quantization process.
The following treatment allows the calculation of the cross-section for a multi-level
molecule by time-dependent perturbation theory. The hypotheses are the
assumption that the incident beam is weak enough to be considered a perturbing
element of the Hamiltonian, and that the broadening of the energy level is negligible.
(1.48)
37
Fig. I.5. Feynman diagrams of the two channels involved in the quantum description of Raman
scattering: the arrows describe the photons created or annihilated during the event, whereas on the
horizontal line the sequence of the molecule states involved in the transition are reported.
The transition rate (1/τ) for a process in which an incident photon of energy ω is
destroyed and another one of energy ωs is produced is calculated according to the
perturbation theory, arresting the expansion of the probability to the second order:
this quantity corresponds to the transition probability between two states m and n,
divided by time. The global transition rate for the scattering phenomenon is
summed over all the possible final states: moreover, in the first passages the
contribution of all the possibly involved phenomena are considered.
ℋ
ℋ ℋ
The expression contains both the first and the second order terms of the transition
probability and it is shown to be dependent only on the perturbation Hamiltonian
ℋi = ℋED. The first term inside the modulus reproduces the Fermi golden rule
expression and provides the rate of first-order transition form m to n; the second
(1.49)
38
term provides the indirect transitions from state m to state n via a range of virtual
intermediate state u [I.16].
A general scattering event does not involve a single mode of the radiation field, but
the creation and the destruction operator affect different modes of the
electromagnetic field: thus, it is necessary to introduce â†, â, â†s,âs. A quantum state
describing the interacting system is indicated by the bra |l, ls, i> where the first two
letters are the number of photons of the incident and the scattering fields
respectively, while the third indicates the molecule energy level. Adapting the
equation 1.49 for the transition rate to new notation, the expression for an initial
state of l incident photons and the molecule in the ground state (m = 0) results4 in
, , ℋ , , ℋ , ,
This kind of equation belongs to the class of integral equations that give the
solutions for quantum mechanical problems of scattering theory [I.18]. The second-
order transition rate can be simplified and a more explicit expression shows the two
concurring paths for the interaction of the two photons:
τ
πe ωωs3l
s nu um
ωu ω
nu s um
ωn ωu
ω ωs ωnm
ksn
where , s are the unit polarization vectors of the incident and scattered photons
and Dnm is the matrix element m|D|m . This expression correctly predict the
dependence on the third power of the scattered pulsation, which, multiplied by the
angular frequency of the incident wave, recover the fourth power typical of the
4 A more rigorous form can be found in the 2nd edition of Loudon [I.16]: the presence of the nonlinear Hamiltonian gives rise to an additional term inside the square modulus. The first term at the right hand side of the equation corresponds to a non linear event which destroys a photon k and creates ks: the Hamiltonian in this case is proportional to A2[5]. The second term (proportional to Ap) is implicitly made out of two contributes which differ in the type of the intermediate state l: one produces the operators in the order âs
†â, the other â, âs†. Separately the two contributes do not
conserve the energy, but their combination does, so can it be accepted; in the time between the two events the molecule belongs to a state l which is different from both the initial and the final state. Due to the relationship B2 = E2/c2, the nonlinear term can be neglected in most cases (when the denominator in the second term is different from zero).
(1.50)
(1.51)
39
scattering events.The transition rate can be converted to a cross-section by dividing
it for the flux density c/V
This expression, which was obtained first by Kramers and Heisenberg, is suitable for
describing both Rayleigh (m = n, and Thomson, for high frequency) and Raman
scattering. The summation is limited to ωf < ω so that the delta function is not
needed but the conservation of energy requirement is automatically fulfilled.
Complete formula takes into account the two independent photon polarizations
[I.16]. Both this equation and the semi-classical formula obtained by Placzek [I.14]
provide a general framework, and can be simplified according to the range of
energies involved by the scattering, or to the kind of molecular functions involved
(purely vibrational, vibronic, etc.).
General considerations.
- Raman scattering is much less effective than the elastic scattering, which normally
regards a small fraction (10-3, Raman scattering Theory, David W. Hahn) of the
incoming photons. Thus, high intensity light source are required for observing it.
Another strict constraint is, naturally, the monochromatic character of the exciting
electric field. For best resolution performances, a narrow emission-line laser is the
choice of preference.
- Raman spectra provide the same kind of information of IR absorption spectra, but
they obey to different selection rules: therefore, in many cases the two techniques
work in a complementary way to characterize the structural and chemical
properties of a material.
- Stokes branch is more intense than anti-Stokes: the main reason is
thermodynamical, and a proper evaluation of the ratio between symmetric bands
can be obtained with the quantum mechanic treatment.
- Vibrational spectrum are generally reported in terms of the relative shift,
expressed in wavenumbers or inverse wavelengths, between the energy of the
detected photon and the one of the exciting photon. The most common unit for the
inverse wavelength coordinate is the cm-1. This allows an easy comparison not only
(1.52)
40
among spectra of the same method obtained with different excitation wavelengths,
but also between Infrared and Raman spectra of the same material, despite
corresponding to different techniques, can be put side by side. On the other hand,
one must not forget that the spectral extension of the spectra is, in the absolute
frequencies scale, much different, with evident consequences on the potential
resonances effect of the chosen source of radiation and on the sensitivity of the
detector. If, for example, the N2 vibrational mode is considered, corresponding to
2331 cm-1, this will be found at 387 nm if the exciting wavelength is 355 nm; if,
instead, the incident wavelength is 632 nm, the mode will be shifted at 741nm [I.19].
- Even if only a full reconstruction of the vibrational levels of the molecule can
provide the correct description of every spectral feature, in many practical uses
Raman spectroscopy can be set aside by an extensive approach. In many molecules,
indeed, atoms can be grouped in sub-units which often possess their own vibrational
modes that are not strongly affected by the global geometry of the molecule. On the
basis of this consideration, it is possible to report in tables, now available for many
class of materials, the typical energy interval in which the vibrational mode
involving the sub-group can be found. An example is shown in figure I.6.[ I.3]
- Since Raman spectroscopy traditional probes use light sources in the visible or
near infrared wavelength range, Raman scattering is not the only form of radiation-
molecule interaction. On the contrary, it is much likely that the material shows
absorption for the chosen wavelength, and therefore luminescence (excitation of
electronic upper energy levels, followed by a radiative decay) is often a competitive
phenomenon for Raman. Different approaches have been proposed and adopted to
overcome, or at least to limit this problem: the last paragraph of this chapter
describes Surface-Enhanced Raman Spectroscopy as an increasingly convenient
option in this direction.
- The treatment reported here below does not consider the angular dependence of a
Raman scattering event. While useful consideration could be drawn from this
description, introducing the formalism needed for this part of the problem will
exceed the scope of this thesis. We refer to Griffiths [I.20] and to Sakurai [I.21] for a
complete theory of scattering.
41
Fig. I.6. Energy distribution of the most common vibrational modes in the spectral region 0-700 cm-1
[I.3].
I.4 The cross section.
Experimentally, the quantity that can be revealed by a detector of electromagnetic
radiation is the intensity; it is convenient, therefore, to quantify the probability that
a Raman event takes place not in terms of the scattered field, but of its square
modulus. Indeed, the classical expression [I.10] for the intensity associated to a
radiating dipole, along a direction which creates with the dipole p an angle ϑ is
IS = ωS4 |p|2 sin2ϑ /(32 π2 ε0 c3)
Where the temporal variation of p is averaged over an oscillation cycle. This quantity
can be also written in terms of the scattering direction, represented by the unit
vector eS
(1.53)
42
IS = ωS4 |eSp|2 /(32 π2 ε0 c3)
There is a way to correlate the intensity of the scattered field with the one incident
on the area of interest: cross section (σ) gives at a glance an indication on the
efficiency of the considered scattering process. Loudon defines σ as the rate at which
energy is removed from the incident beam by scattering, divided by the rate at
which the energy in the incident photon beam crosses a unit area perpendicular to
its propagation direction [I.16].
σ ωs
ωI Isr
d
In case of Raman scattering, the value of σ is not only related to the exciting laser
wavelength, but to a particular vibrational mode of the selected molecule of angular
frequency ω – ωs. This quantity can be expressed in terms of the transition rate τ of
a scattering event, provided that the volume V which participates to the scattering is
well defined as the product of the cross section times the length crossed in that time
by the light in the material, nk c τ.
A differential cross section, dσ/d can be introduced when the cross section angular
distribution is of interest: this is often the case for an electric dipole, where the
scattered radiation is not isotropic. A possible definition for the differential
scattering cross section is given by Cardona, as the ratio between the energy emitted
per unit time by an electric dipole M and the energy incident on that dipole divided
per unit area and unit time, [I.22]
dW = d |es α el|2 EL2ω4/(4π)2 ε0c3
by the energy incident on that dipole per unit area and unit time, W = ε0c EL2, and
integrating over the solid angle ; this definition can be proven to be equivalent to
the. The unitary vectors el and es respectively refer to the polarization of incoming
and scattered of (laser) light. The expansion of the polarizability carried out in 1.5
easily leads to an expression for the Raman component of the scattering cross
section. In equation I.56 the differential cross section for a Stokes-shifted line at
angular frequency ωs = ω0 – ωk is reported. [I.5, I.11]
dσs/d = |es α/ Qn el|2<QkQk*> ωs4/(4πε0)2c4
where < > represents the thermodynamical average over the ground state of the
molecule [I.22], needed to take into account the different population of the
(1.54)
(1.54)
(1.55)
(1.56)
43
vibrational levels in an ensemble of many molecules. This formula closely resembles
the intensity formula (1.37) obtained by the semi classical theory, and reveals the
explicit dependence of the polarizability tensor on the normal coordinates Qk.
I.5 Surface Enhanced Raman Scattering.
Though Raman spectroscopy gives detailed chemical and conformational
information, the small scattering cross-section has limited widespread use.
Experiments performed in the mid 1970s demonstrated that molecules adsorbed to
a roughened metal surface generated anomalously large Raman intensities [21]. This
phenomenon is known as Surface-Enhanced Raman Scattering (SERS), where the
last S can also be used to refer to Spectroscopy, where the attention is given to the
technique more than to the effect exploited. Enhancements varying from 103 to
1011[I.23] have been reported for molecules adsorbed to nano-structured silver,
gold and copper, in order of width of use, but other metals have found application in
minor cases. While there is still occasion to debate about a commonly accepted
theory of the phenomenon, general agreement is given to the attribution of the main
reason for this boost in the Raman cross section to a so-called Electromagnetic
Mechanism (EM). Occasionally, this factor can be helped by a Chemical Mechanism
(CHEM), which nonetheless is of lesser importance.
Electromagnetic Mechanism is mostly related to the excitation of a localized surface
Plasmon resonance by the laser source. Briefly, the nanometric features of the metal
substrate on which the molecule is adsorbed are characterized by collective
oscillations of charges (typically conduction electrons), which can be selectively
e cited by resonant laser wavelengths. These “plasma waves” are not only localized
inside the roughness features of the conductor, but naturally they are confined to its
surface: hence comes the name of Surface Plasmon Polaritons. This allows the
Raman cross section of the modes of the adsorbed material, which are parallel to the
excited plasmons, to benefit of the huge electric field which is localized along the
metal surface. CHEM enhancement, instead, is not only site-specific but it also
depends on the analyte: it is present when a charge-transfer state is created
between the metal and the adsorbed molecule. If the laser wavelength is not only in
resonance conditions with the metal nano-features, but with an electronic transition
44
of the molecule under analysis, the effect experiences a further enhancement and it
is called SERRS, where the first R of the acronym stands for Resonance.
The character of resonance technique is, however, implicit in the description of the
Surface-Enhanced Raman effect: for this reason, even if the enormous gain given to
the signal to noise ratio of the vibrational spectrum makes this technique preferable
for samples in very low concentrations, or for cases in which fluorescence would be
an unavoidable obstacle, some caveats must be considered whenever a SER analysis
is planned. First of all, the enhancement provided by the interaction with the
plasmon is naturally very selective: not all the vibrational modes are affected in the
same way, but, as previously reported, geometry plays a fundamental role in
determining the effect, due to the relative orientations of the vibrational modes with
the excited plasmons, the polarization of the incoming field, the distance between
the roughened surface and the different parts of the molecule, etc. Without going too
much into details, these variables result in a distortion of the SER spectra with
respect to the normal Raman ones, which can be traced in terms of a different
intensity ratioes between the peaks or, if the local environment of the molecule has
significantly changed, in broadening or shifts of the vibrational features. It must be
noted, moreover, that there does not exist a perfect SER substrate, which can be
used for every sample, but different materials and shapes produce variable effects
according to the wavelength of the chosen laser and, of course, to the analyte.
Nonetheless, the study and the exploitation of SERS are growing: in the last ten years
the number of published works dedicated to or containing the SER technique more
than doubled, and the trend does not seem to decrease [I.24]. The development and
consequently the availability of cutting-edge methods permits the researcher to
adopt an increasing number of possible geometries, shapes of the structures,
materials and, in general, probing methods. If the stability still makes the traditional
silver or gold nanoparticles a reliable starting point for a SER measurement, the
current tendency is to design the substrate parameters for a particular analyte,
making SERS a truly tailored detection and identification method.
45
Bibliography.
[I.1] A. Smekal, Naturwiss. 16, 873 (1923);
[I.2] C.V. Raman and K.S. Krishnan, Nature, 121, 501 (1928);
[I.3] E. Smith, G. Dent, Modern Raman spectroscopy: a practical approach, John Wiley
& Sons(2005);
[I.4] I.R. Lewis, H.W. Edwards. Handbook of Raman Spectroscopy. From the Research
Laboratory for the Process Line, CRC Press (2001);
[I.5] R. Aroca, Surface Enhanced Vibrational Spectroscopy, John Wiley & Sons
(2007);
[I.6] N. Ashcroft, M. David , Solid State Physics, Cengage Learning Emea (2000);
[I.7] E.B. Wilson, J.C. Decius, P.C. Cross, Molecular Vibrations: The Theory of Infrared
and Raman Vibrational Spectra, Dover Publications (1955);
[I.8] D.C. Harris, M.C. Bertolucci, Symmetry and spectroscopy: An Introduction To
Vibrational and Electronic Scattering, Dover Publications (1989);
[I.9] G.Moruzzi, Dispense di struttura della materia. University of Pisa
[I.10] P. Mazzoldi, M. Nigro, C. Voci, Fisica – Volume 2: Elettromagnetismo – Onde,
Edises (2000);
[I.11] E. Le Ru, P. Etchegoin, Principles of Surface Enhanced Raman Spectroscopy
and related plasmonic effect, Elsevier Science (2008);
[I.12] D. A. Long, The Raman effect. A unified treatment of the theory of Raman
scattering by molecules, John Wiley & Sons (2002);
[I.13] W. Demtröder, Laser Spectroscopy - Basic concepts and instrumentation,
Springer (1996);
46
[I.14] Placzek, G. Rayleigh-Streuung und Raman-Effekt, in Handbuch der Radiologie,
E. Marx (ed.), 6, 205–374. Academische Verlag: Leipzig (1934);
[I.15]W. H. Weber, R. Merlin, Raman Spectroscopy in Materials Science, Springer
(2000);
[I.16]R. Loudon, The quantum theory of light. Second edition, Clarendon Press,
Oxford,(1983);
[I.17]H.A. Szymanski, Raman Spectroscopy: Theory and Practice, Plenum Press,
(1967);
[I.18] E. Merzbacher, Quantum mechanics, 3rd edition, John Wiley & Sons (1998);
[I.19] David W. Hahn, Raman Scattering Theory, University of Florida (2007);
[I.20] D. Griffiths, Introduction to Quantum Mechanics, Prentice Hall, (1995);
[I.21] J. J. Sakurai, Modern Quantum Mechanics, Yoshioka Shoten, Kyoto, (1989);
[I.22] M. Cardona, G. Guntherodt, Light Scattering in Solids, Vol. 2, Basic concepts
and instrumentation, 3rd edition, Springer (1989);
[I.23] R. P. Van Duyne, C. Haynes. Raman Spectroscopy, Northwestern University
(review available online);
[I.24] B. Sharma, R. R Frontiera, A.I. Henry, E. Ringe, R. P. Van Duyne, SERS:
Materials, Applications, and the Future Surface Enhanced Raman Spectroscopy,
Materials Today, 15 (2012), 16–25.
47
CHAPTER II
THE REMOTE RAMAN SCANNER.
The determination of the physical processes resulting in a Raman scattering event,
carried out in the first chapter, enables the researchers to consider all the necessary
parameters in the preparation of an experiment. It is even more crucial, when
designing a novel instrument which relies on this effect, to determine the physical
quantities it involves, and hence the most suitable techniques for the detection of
this precious but weak signal, the critical points and the advantages of the possible
approaches and the recent discoveries and innovative methods concerning Raman
spectroscopy. This chapter focuses on the development of the Remote Raman
Scanner instrument, starting from its objectives to the phases of the project to the
construction. An introductory section, however, is dedicated to the application of
Raman spectroscopy to the field of Cultural heritage, in order to appreciate in which
direction the proposed device should be situated.
II.1. Raman spectroscopy in Cultural Heritage.
Identification of materials in and on objects of cultural and artistic interest has long
been recognized as a task necessary for uncovering the history of such objects and
finding out possibly how, where and when they were made, what was their use and
even how they have interacted with their environment during their lifetime.
Furthermore, knowing the materials not only opens a window to the past for
archaeologists and historians but also enables conservators to pave a safe way to the
future by means of proper preservation [II.1]. The main challenge in this type of
work is the vast diversity and variety of materials encountered, which include:
pigments, mineral or organic, natural or synthetic; metals or metal alloys and their
corrosion products; stone and glass; bio-organic materials such as wood, leather,
48
paper, parchment, but also oil, protein or sugar-based binding media and glues and
synthetic or natural varnish coatings and associated by-products arising during their
aging [II.2]. In this context, Raman spectroscopy proves to be an effective option,
providing a deep insight on the molecular [II.3] and structural [II.4] properties of a
material without altering or damaging it. As an optical measurement, it does not
need any contact between the probe and the sample and the stimulation of scattered
light does not imply high light intensities, so the power of the exciting
electromagnetic field can be kept well below the threshold of polymerization,
ablation or burning, with respect to the possible risks concerning different
materials. The detection of highly specific fingerprints such as the frequencies of the
vibrational modes enables the researchers to distinguish among similar materials
and even among different crystal phases of the same compound, such as in the case
of minerals; moreover, the vibrational frequencies depend on the strain undergone
by a solid sample, so they can be used as a stress indicator (showing deformations
before they become irreversible); furthermore, the influence of thermal energy on
the ratio between the Stokes and anti-Stokes spectral branches, can be measured to
monitor the temperature evolution of a sample, for example due to exposure to the
laser beam [II.5].
A huge number of publications attests in the last 20 years the widespread
possibilities of employing Raman spectroscopy on objects of art such as paintings
[II.6], frescoes [II.7], drawings [II.8], mosaics [II.9], sculptures [II.10], textiles [II.11],
illuminated manuscripts [II.12], old prints [II.13], parchment [II.14], miniatures
[II.15], but also on pottery [II.16], porcelains [II.17], coins [II.18], jewels [II.19],
human and even feline mummies [II.20,II.21]! ssessment of an artwork’s
conservation state and of the validity of its restoration; or interpretation, dating and
etiology of a controversial artifact; these are all examples of case studies which
benefit of this incredible source of information.
Of course, Raman spectroscopy alone is not generally sufficient to provide a
evidence to every identification problem, but it is usually employed together with
other non-invasive (IR spectroscopy, fluorescence spectroscopy, X-ray spectroscopy,
etc.) or micro-invasive methods (laser-induced breakdown spectroscopy, gas
chromatography-mass spectrometry) in order to obtain complementary
information. As explained in the previous chapter, indeed, Raman spectroscopy is
49
based on a rather weak effect, and detection of the materials’ spectral fingerprints is
often hampered by the presence of a high fluorescence background signal. This is
particularly true when the sample is of biological origin, like binding media,
varnishes and dyes in the application to artworks. Raman spectroscopy, however,
has several advantages (rapidity, possibility to be performed in situ, no need for
sample preparation) which frequently make it preferable even to more “efficient”
techniques: in particular, because of these features it is an ideal preliminary method,
useful to restrict the range of possible answers to an identification, before more
tailored, but possibly more invasive experimental techniques are considered.
II.2. The aim of the project.
The proposed instrument must conjugate some of the most important features for
the analysis of valuable (and sensitive) objects. It is going to be operated, indeed, by
a research group whose primary activity is the study of objects of artistic or
archaeological interest [II.22], together with other already available techniques
[II.23-II.25]. Raman spectroscopy, as previously stated, is one of the favored
techniques to collect molecular information from this kind of materials.
In such delicate applications it is particularly relevant that the analysis method is
non-invasive: this requirement is more restrictive than non destructivity, since it
implies that the experiment does not affect the integrity of the sample and possibly
does not interfere with the ambient conditions in which it is kept [II.26]; for Raman
spectroscopy, this necessity often means that the contact or proximity approach are
not enough, but in many cases a certain distance between the instrument and the
analyzed surface is required to preserve the physical, chemical or biological
environment of the object of interest (e.g., a fresco in a narrow niche, an ancient
scroll under a controlled atmosphere, a mural frieze in a cave).
Remote analysis, in addition, can be integrated with another desirable capability for
the instrument: the possibility to analyze an extended area of the target surface
without moving the sample. In the study of Cultural heritage, indeed, a punctual
analysis is rarely significant for the entire object, and therefore a meaningful Raman
analysis implies either to extract several samples from the studied item, or to shift
the Raman probe at different positions over its surface. Such a feature, therefore,
50
would be essential, not only to expand the sampled area of a target material, but it
could also foresee application on bulky or precious artifacts for which analysis is
often prevented by practical impediments connected to the impossibility of being
moved.
This requirement is directly related to the third one, which is the transportability.
The already mentioned reasons are driving forces towards an instrument with
compact size and limited weight, which could be easily carried in a museum, a
cathedral or an archaeological site. The planned Raman instrument is accordingly
designed to work as a transportable remote imaging spectrometer: the imaging
method, as explained in the next sections, involves the acquisition of a Raman
spectrum from different points of a surface, and the spectra are combined together
after the measurement.
Before engaging in the project of a system, though, it was important to explore and
compare the range of solutions offered by already existing devices, commercial or
developed by other research groups, designed for similar purposes. A brief report of
the available techniques of Raman imaging, remote and in situ Raman analysis is
given in the next paragraph, with a particular attention for applications in the
Cultural heritage field.
II.3. The state of the art.
Raman imaging.
Raman imaging can be implemented with two different approaches: direct Raman
imaging and Raman mapping. In direct Raman imaging, the laser spot is defocused in
order to illuminate a relatively large sample area, and an image detector, coupled
with suitable filters, is used to acquire images at specific Raman shift frequencies (or
wavenumbers). For the purpose, dielectric [II.27, II.28] and acousto-optic or liquid
crystal filters [II.29-32] are most often employed. The use of a single dielectric filter
integrated with a tunable laser has also been proposed [II.33]. The direct approach
has the great advantage of being faster than Raman mapping due to the parallel
acquisition provided by a wide field imaging detector. Nevertheless, the intensity of
51
the collected Raman signal can be very low due to the need for defocusing the laser
beam and to the attenuation factor of filters. As a consequence, direct Raman
imaging is typically limited to microscopy applications, the width of the field of view
being of hundreds of microns, and is especially useful when a priori information on
the analyzed surface is already available, allowing one to investigate few selected
spectral Raman bands [II.34]. In contrast, in the Raman mapping approach a Raman
image is generated by performing a serial acquisition of many points in the area of
interest. With this method, when the laser is focused on a spot (point mapping), the
information is reconstructed by sequential single-point acquisitions at each x, y
position with a suitable Raman spectrometer. In contrast, with line mapping the
laser is focused onto a line and a bi-dimensional detector, coupled with a dispersive
element, is used to register both the spatial and the spectral information of the
Raman signal produced along the line [II.35]. Generally, the line mapping approach
is preferable to the point mapping approach, thanks to a lower acquisition time and
higher SNR.
An algorithm introduced by Puppels et al. [II.28], estimate the signal to noise ratio
for both Raman imaging and mapping, and therefore helps to determine the best
option with respect to the theoretical experimental parameters (exposure times,
number of pixels of the detector, readout noise): this method, however, is hardly
applicable to real case studies, because of the non-uniform frequency response of
the filters and the detectors, and the difficulty in quantifying the terms introducing
losses in the signal collection.
For the analysis of art, Raman mapping proved to be particularly advantageous,
since it provides high spectral resolution. For example, recent works have
highlighted the capability of Raman mapping to analyze polished cross sections of
paint layers [II.36,37], to evaluate the penetration depth of inorganic and organic
substances in conservative treatment [II.38], as well as to study the yellowing effect
of laser cleaning treatments for the removal of black crusts from stones [II.39]. In all
the reported cases, however, the size of the analyzed area is never bigger than
1 mm2[II.37, II.40].
Remote Raman sensing.
52
Here, and in the rest of this work, the term “remote” is adopted to indicate
instruments which are kept at a certain distance from the sample under
investigation, and not to the devices which can be controlled by far, such as the
Raman spectrometers for oceanographic studies [II.41]. The former, which are also
called stand-off spectrometers, usually perform Raman spectroscopy at a distance of
the order of tenths of meters [II.42]. If its principle was first proposed in the mid-
1960s, only thirty years later the technology was mature enough to permit the first
measurements, carried out on atmospheric phenomena [II.43]. Ranged
measurement are generally favorable over proximity analysis because, when
performed in situ, they suffer less from vibrations and other stability issues. of
course increasing the working distance [II.44]. Naturally, the increased focal length
generally implies a lower acceptance angle for the collection optics, and as a
consequence the signal intensity is considerably reduced. Nonetheless, the adoption
of powerful solid-state laser sources (preferentially frequency-doubled Nd-Yag,
[II.45]), typically working in pulsed regime, is sufficient to provide qualitatively
good spectra from samples which do not risk to be damaged by high energy pulses.
The collection of the scattered light exploits casse-grain telescope objectives, which
can be directly coupled to spectrograph or to acousto-optic tunable filters (AOTF),
or connected by optical fibers to the detection apparatus. One of the reported
devices is also able to work in a scanning mode, thanks to a two-axis motorized
motion of the prisms which deliver the laser beam inside the telescope [II.45], still
no evidence of the effectiveness of this approach has been published yet.
These instruments, however, are generally conceived for the remote analysis of
dangerous materials such as explosives [II.46], or samples in difficultly reachable
positions, like rocks or even clouds. Their working distance is at least of the order of
the tenths of meters (it has been driven up to 533 m [II.45]), and therefore they find
little application to the study of Cultural heritage. Currently, no intermediately
ranged instrument is available, neither as a commercial device, nor as a one-off tool
built by a research team. A short range approach, however, has been chosen by
Vandenabeele et al. [II.47] for the design of the first Cultural-Heritage-oriented
Raman spectrometer, called MArtA (Mobile Art Analyzer): the instrument is
portable, and its working distance can be adjusted up to 2.5 cm, settling it out of the
standard micro-Raman set-ups. A more thorough report about its performances is
53
given in the following section; its focal length, however, can be considered to
determine the order of magnitude of the longer working distance currently available
for a Raman instrument not based on a telescope reflector.
Portable Raman instruments.
In the last ten years, the availability of robust, air-cooled laser sources, the
miniaturization of detectors and their electronics as well as the lap-top computer
increase have led progressively to the development and use of more and more
compact Raman set-ups: transportable, at first, then mobile (< 30 kg) and even
hand-on (< 2 kg at least for the remote head) ultramobile spectrometers are now
available [II.48]. Generally speaking, laboratory equipment still performs better than
mobile Raman instrumentation. It is clear that during the design of the mobile
instrument some concessions have been made in order to create a compact and
stable Raman spectrometer. Besides, non-mobile dispersive Raman instruments are
usually equipped with multiple lasers, allowing the researcher to select the most
appropriate laser wavelength for the investigation on hand. Moreover, laboratory
instrumentation is in general well positioned in a dark air conditioned room on a
solid laboratory table, guaranteeing optimal alignment conditions and a high
throughput of light [II.48]. Nonetheless, industrial manufacturers and specialized
research groups spend many efforts in the development of increasingly effective
portable Raman spectrometers, because the potential fields of application are
enormous: not only Cultural heritage, but also geosciences [II.49] and forensic
science [II.50], just to cite three of the sciences which have already started to benefit
of these instrumentations.
Among the stand-off instruments, the prototype built by Vandenabeele, MArtA,
which exploits a 785 nm diode laser was cited. This instrument, in which a probe
made out of a bundle of 37 optical fibers is equipped with a interchangeable focusing
lens, the focus being helped by remote-controlled micro-positioners [II.51]. MArtA
proved to be efficient over quite a wide range of materials, from Egyptian sarcophagi
to paintings on paper or wood, to mediaeval frescoes [II.51] a comparison with
mobile commercially-available Raman spectrometers has been carried on by
Vandenabeele itself, with a positive validation [II.52]. Another portable Raman
device was adopted by C. Miliani et al., and is one of the numerous analytical
54
methods available on the Mobile Laboratory (MOLAB) of the Perugian research
group [II.53]: this is however, one of the first commercially available instruments, a
Jasco RMP-100 microprobe, equipped with an Olympus objective (50× or 20×), for
a total weight of 25 kg. This instrument allows measumrement of areas of the order
of 5 × 5 µm2 approximately [II.53]. A completely different approach has been
followed by R. Ernst for the development of his spectrometer, based on a Senterra
Raman microscope which is mounted on a transportable gantry: this frame supports
the microscope probe, allowing it to be translated over large flat samples (up to 100
× 70 cm2). This instrument has been successfully applied in situ for a series of
measurement on Mongolian thangkas [II.44] and it is surely very suitable for
monitoring wide objects such as paintings, but it cannot perform analysis without
removing them from their original vertical position. Moreover, its structure does not
allow analysis of three-dimensional objects: the vertical translation stage allows
very precise focusing but it does not permit wide excursions from the default
distance .
Since the first pioneering attempts, new portable Raman spectrometers have been
introduced by the the researchers and by the manufacturers, resulting in a wide
range of commercial and custom instruments which are finding an extending
application also in different fields from archaeometry and conservation. For
example, a challenging and growing potential application of this technique is to take
part in a future mission to Mars.
The preferred choice for the laser sources used by these devices is the diode laser
emitting at 785 nm, closely followed by the Neodimium: Yttrium Aluminum Garnet
(Nd-YAG) frequency doubled at 532 nm: these two options, indeed, offer relatively
cheap solutions, with the significant advantage of a robust and not-cumbersome
packaging.
The great majority of the reported mobile devices are able to perform meaningful
spectral analysis in a dark environment, because they suffer from stray light noise:
therefore, either they require the room which hosts the object of interest to be
obscured, or, for instrument with a compact probe head, they need to apply a black
coat around the analyzed area to screen the surrounding illumination.
55
II.4. Remote Raman Scanner: the layout.
In the application to artworks and archaeological finds, thus, the mainstream is to
perform Raman measurements with a mobile instrument, which relies on a
traditional microscope layout or is equipped with a fiber connected probe, whose
working distance is of the order of tenths of millimeters in the best case. All the
reported instruments, consequently, suffer from instable supports: vibrations occur
very frequently when the measurement is performed in situ, and as a result the non-
perfect focus of the laser beam affects the quality of the spectra. This issue must be
generally assigned to the difficulty in reaching the desired area of the object of
interest in environments that have not been built according to this purpose.
Insensitivity to slight focus variations and a longer working distance can actually
help the on-site monitoring of Cultural Heritage, by reducing the set-up times for
the measurements, but, most of all, enabling the analysis of otherwise off-limits
specimens.
For this reasons, the project choice for the Remote Raman scanner was to design a
stand-off spectrometer able to work at an intermediate distance between traditional
Raman devices and the spectrometers for the remote analysis; therefore, it does not
rely on a microscope objective or a casse-grain layout, but on a custom lens-built
optics with a focal distance of at least 20 centimeters [II.54]. The capability of
performing a Raman analysis of a wide area is obtained thanks to two factors: the
field of view is widened by the choice of a long-working-distance optic, and the
selection of the focused point within the field of view is performed by a deflection of
the laser beam. The last feature is achieved by inserting in the light path a couple of
orthogonal galvanometric mirrors, which tilt of an arbitrary angle the reflected
beam (within the allowed range) respectively along the x and the y Cartesian axis of
the focal plane. The presence of these two additional degrees of freedom in the light
path introduces the task of determining the suitable optics to correctly focus the
laser beam at the chosen focal distance for any angular shift provided by the
mirrors. This requirement would not be particularly challenging, if the same optics
weren’t used for the collection of the scattered light as well. The geometrical
configuration selected for the device is, indeed, indicated as “backscattering mode”:
the optical axes referred to the beam, before and after the scattering event with the
56
target material, are disposed with an angle of pi (180°) with respect to each other.
Naturally, this implies that the optics which is responsible for the collection of the
Raman signal must be the same which focuses the excitation laser beam. More
details on the optical system are reported in a dedicated paragraph.
The design of the instrument determined other relevant choices for the project: a
semiconductor laser, with an external cavity configuration, emitting at 785 nm, is
used as the light source; a cooled Charged Coupled Device (CCD) sensor is adopted
as the detector of the scattered light; dispersion of the spectral components of the
Raman signal is provided by a single-turret Czerny-Turner spectrograph, while
rejection of the elastic scattered light is assured by a dichroic filter and a notch filter,
centered at the laser emission wavelength; connection of the laser source with the
optical system, and from the latter to the dispersing element and the sensor, relies
on optical fibers, coupled with collimating lenses. Minor specifications about the
instrument set-up are given in the next sections: it is worth noting, however, that a
consistent part of the project has been the development of a specifically-thought
unified software control, which provides the interface for the user of the Remote
Raman Scanner in order to manage the available experimental parameters and to
monitor and save the results of the analysis.
The definitive version of the instrument can be seen in figure II.1: the laser source
and the detection stage are lodged on a dedicated scaffold (transportable by a
trolley), and two optical fibers (3-meters long) are used for connecting them with
the proper probe head, built on a carbon fiber reinforced plastic breadboard and
mounted on a photography tripod. This part of the instrument hosts the optical
system, which, as previously stated, focuses the light incoming from the laser
through the first fiber, and deliveries the collected backscattered light to the second
fiber, which drives it directly to the spectrograph entrance slit. The two optical
paths, which join inside the optical system, are separated by a dichroic mirror, which
reflects on a perpendicular direction the electromagnetic radiation whose
wavelength is exactly 785 nm and is crossed by the higher spectral components. In
this way, the incoming laser beam is deflected towards the optical system, while the
returning light, backscattered by the sample, is separated in frequency. The elastic
component is reflected, while the Stokes component of the Raman scattering is
57
transmitted towards a notch filter (who further rejects the remaining laser line) and
coupled to the second fiber.
To our knowledge, this is the first Raman spectrometer which exploits a pair of
galvanometric mirrors to perform a dynamic map of a remote surface under
investigation; it is worth to notice that, even if the instrument described and built by
Puppels et al [II.28] adopts a similar scanning system, that is actually a Raman
imaging device which takes advantage of the periodic movement of the
galvanometric mirrors to produce an homogeneous illumination of the field of view.
Figure II.1. The layout of Remote Raman scanner. From left to right, the computer control, the
detection unit and the laser, lodged on a trolley, and the remote probe, positioned on a tripod in front
of the tripod.
II.5. RRS: the standard components
Semiconductor laser.
The adopted laser source is the Lion model, produced by Sacher Lasertechnik GmbH
(Germany). It is a small (165×60×54 mm3), light (0.6 kg) semiconductor laser,
working in continuous wave (CW) regime (figure II.2) and equipped with a Littman
external cavity: this configuration exploits a diffraction grating as one of the cavity
folding mirror. This element, illuminated by the laser emission through a collimating
lens, provides a spatial dispersion of the emission modes of oscillation of the laser
cavity, so that only the radiation of the chosen wavelength can reach the lasing
threshold. Mode hopping and frequency drift, typically related to semiconductor
58
lasers, are therefore suppressed: additionally, the high quality of the cavity
elements, together with a special anti-reflection coating of the exit surface, grant a
spectral width of only 500 kHz and a maximum output power of 270 mW [II.55].
The laser head is driven by a remote control (Pilot) which manages both the current
supply and the temperature control of the device: it is important, for the stability of
the light emission and the durability of the laser diode, that the temporal behavior of
these two parameters is smoothly varying and a continuous check of the status of
the light source is given as a feedback to the Pilot.
Fig. II.2. Layout of the Littman cavity laser. The active medium (in pink) is crossed by the laser beam
focused by two lenses (L1 and L2). The first lens collects only the emitted light which bounces back
from the mirror M, according to the selection performed by the diffraction grating G. Thanks to this
element, only radiation at very narrow wavelength can reach the laser threshold and leave the cavity
through lens L2.
The wavelength for the excitation of the Raman effect lies at the lower border of the
Near Infrared (NIR) range. This choice has been made in order to limit the possible
luminescence emission by the target material, which in many cases overwhelms the
much less effective Raman signal. Most of the luminescent transitions are, indeed,
triggered by radiation in the Ultraviolet (UV) or visible wavelength range. There are,
however, a number of drawbacks related to the adoption of a NIR laser source. First
of all, the quantum efficiency of a traditional silicon sensor decreases for
wavelengths above 700 nm; moreover, the non-resonant Raman cross section was
shown to be inversely proportional to the fourth power of the wavelength. However,
an excitation wavelength in the UV, which provides the maximum efficiency, does
not match the commonly available optical components, and therefore would have a
59
negative influence on the overall budget for the instrument. Additionally, the
spectral resolution of a Raman spectrum, ceteribus paribus, increases with the
wavelength; furthermore, a laser emitting in the UV or in the visible range results in
higher absorption rates by the observed samples, which enhances the risk of
photochemical or thermal degradation. For this reason, moreover, a CW laser has
been chosen, instead than a pulsed source. Even if the Lion® can provide quite a high
intensity, it should be noted that this extra power is needed to compensate the
losses introduced along the beam path by the optical fibers and the set of lenses. As
will be stated in the next chapters, though, the power density which was actually
delivered on the sample has always been kept within a safety limit (< 400 W/cm2).
Galvanometric mirrors.
The Remote Raman Scanner employs a VM1000+ (Cambridge Technology, USA)
galvanometric system for the deflection of the laser beam. The device is made of a
pair of mirrors, mounted on two orthogonal axes; each mirror is free to rotate,
within a permitted range, around its axis and its angular orientation is selected by a
current value. This system exploits, indeed, the alignment of a coil in which current
is made flow, with a permanent magnet, driven by the current value; the response of
the mirror, which depends by its moment of inertia, is generally very rapid (down to
0.5 milliseconds) and pretty accurate (the galvanometer can be used as a device to
measure currents down to 1 nanoAmpère). The considered system is designed for
many laser scanning purposes (marking and prototyping above all), and therefore is
not specifically conceived to work in a Raman spectrometer: some of its features,
such as the dimensions of the rotating mirrors (respectively 10 and 15 mm along the
rotating axis for the X and Y deflector), can be limiting in the development of the
planned optical path; nonetheless, the system is sufficiently small not to interfere
with the compact design of the overall probe head. Other features which make this
device compatible with the purpose of this project are its good angular resolution
(2×104 steps per each angle), the angular excursion of 80° along both the horizontal
and vertical axis, and the reflective coating of the mirrors for the NIR range.
60
Holographic notch filter.
The holographic notch filter selectively rejects (through Bragg diffraction) light
falling within a narrow spectral interval, while leaving unaltered the other spectral
components of the electromagnetic radiation which crosses it. It is constructed in a
photosensitive medium, dichromated gelatin, by exposing it to interfering laser
beams, which create a periodic modulation in the refractive index. This periodicity
produces a strong 3d Bragg reflection that can efficiently (> 99.9 %) diffract away
the Rayleigh line, while transmitting adjacent wavelengths with > 90 % efficiency
[II.56].
Being much more economical, practical and smaller than a dedicated
monochromator, the notch filter is the only possible choice to introduce a rejection
element for the elastically scattered light in a portable instrument, with a single
excitation line. Among the commercially available at the time of building the
instrument, the Iridian® ZX000419 notch filter provided the narrowest
transmission curve (with a Full Width Half Maximum of 22 nm) and a considerable
rejection of the elastic component, with an optical density of 4; with a diameter of 1
inch, this element was easily incorporated into the Remote Raman Scanner.
Czerny-Turner spectrograph.
For the dispersion of the spectral component of the Raman signal, the Remote
Raman scanner exploits the SpectraPro2150 (Acton Research Corporation, USA), a
Czerny-Turner (CT) spectrograph: actually, this is the most widely used
configuration for Raman spectroscopy. It makes use of mirrors as collimators in an
off-axis configuration and employs a planar reflective grating in the collimated
space. This design leads to a basic one-dimensional spectral dispersion dimension.
The entering light, in the original design, passes through a vertical slit, whose width
can be regulated by a precision knob.
The principal advantages of the CT configuration are its relative simplicity and
wavelength flexibility. Because it is an all-reflective design, it is naturally achromatic.
The CT is easy to scan and can accommodate multiple gratings, making it an
attractive spectrograph for research systems that require flexibility to operate with
many different lasers. Disadvantages of this design are in the areas of the etendue,
61
imaging performance, durability and thermal/mechanical stability. Vignetting at the
edges of the spectrum is relatively large due to the large distance between the
output collimator and the reflection grating. Thermal instability of the CT
spectrograph is about a factor of 5 higher than that of a similarly configured axial
transmissive spectrograph [II.56].
In the Remote Raman Scanner, SpectraPro2150 represents a trade-off between
performance and limited size, being its internal focal length 150 mm with external
dimensions of 178×178×165 mm. Its weight is just 4.5 kg, which is considerably
helpful for limiting the overall load of the instrument. The gratings mounted on the
single turret are two: they have respectively 600 and 1200 grooves per millimeter,
with a blaze at 750 nm, and can be rotated or interchanged via a stepper rotary
encoder. The first one grants a wider spectral windows, while the latter, which is
used as default, allows for an higher resolution: with the narrowest slit width (10
µm), the discriminating power can be better than 0.4 nm. When employed with the
portable probe head, however, the performance are well below the resolution limits,
due to the intrinsic width given by the diameter of the fiber core, which can be 100
or 200 µm according to the target material’s Raman efficiency: in this configuration,
in fact, the entering slit is represented by the fiber tip, which is plugged to the
spectrograph through a FC port which exactly replaces the original slit.
Charge coupled device (CCD).
Charge-coupled devices (CCD) appeared as reliable, commercial products for
spectroscopic applications in the early 1990s: now, they represent the most
common technology for the detection of light in this kind of experiments. In
particular, this sensor meets more of the desired detector characteristic for Raman
spectroscopy than any other currently available technology. These characteristics
include the ability to measure many wavelengths at once, large dynamic range, low
read noise, low dark current, robust packaging and long detector lifetime. The CCD is
fabricated on MOS (metal-oxide semiconductor) technology. The charge is stored in
the capacitor gate and readout occurs after sequential charge transfers by
periodically controlling the voltages on the electrodes [II.56].
In the ultimate configuration of the spectrometer, a iDus (Andor, Northern Ireland)
front-illuminated CCD is used for the monitoring and acquisition of the collected
62
radiation: it is based on a rectangular silicon sensor of 1024×127 square pixels,
each one with a 26 µm width. The device is equipped with a pre-amplifier and a 16-
bit analog to digital converter and a double-stage Peltier cooling circuit which
permits a refrigeration of the chip down to -70°C in standard conditions. Its
dimensions are 157×100×87 mm3. Whereas a back-illuminated sensor (in which
the chip is flipped upside down and the silicon-active medium is reduced in
thickness such that light enters the silicon from the back side) can be chosen to
enhance the quantum efficiency (QE), the disadvantage of using these types of
detectors for 785-nm-excited Raman is detector etaloning [II.56]. This phenomenon
can be prevented by working in the deep depletion regime, but the dark current
noise is considerably enhanced. For these reasons, and for a considerably lower
price, a standard front-illuminated sensor has been selected. Dynamic range is
generally expressed in terms of the number of bits produced by its digitizer.
However, a significant parameter is the full well capacity of each pixel,
correspondent to the maximum amount of stored charged in each CMOS: in this
particular camera, this value is of 106. The number of the elemental charges is then
read by the digital converter with the possible application of a gain factor; the full
well capacity, however, allows a direct comparison with the typical noise figures of
the sensor, which are also expressed in electrons. In this case, the readout noise is
estimated as 3 electrons, while the dark current is typically of the order of 2×10-3
electrons per pixel per second. under normal conditions, these noise figures are too
low to hamper the detection of the Raman signal [II.55], which is much more
threatened by the competition with luminescence background.
Optical fibers.
Optical fibers provide to the system layout the needed flexibility in order to design a
compact probe head and, at the same time, to maintain a bulkier but high-quality
part for the acquisition and elaboration of the Raman signal. It would be impossible,
indeed, to arrange all the necessary instrumentation on a single transportable
working surface: therefore, some parts of the optical path need to be guided by a
flexible medium. If there is no particular issue for the delivery of the laser beam to
the probe, because the losses can be easily compensated by an higher exit power of
the laser source, introducing losses to the already weak signal is much more
63
disadvantageous. For this reason, a multiple choice for the second fiber, from the
device probe to the spectrograph, is allowed: the main option is a FC-connected,
100 µm core, fused silica, 3-meters long graded-index multimode fiber, equivalent to
the one used from the laser source to the optical system. Its numerical aperture is
0.29. This choice allows a discrete coupling with the backscattered radiation, while
offering a smaller diameter which results in good resolution spectra. If, however, the
collected spectra does not show a sufficient signal to noise ratio, or the exposure
time to achieve an unambiguous spectrum is too long with respect to the
experimental demands, a second option is available: a FC-connected, 200 µm core, 3-
meters long step-index multimode fiber provides a more efficient collection of the
backscattered light, with the drawback of hampering the resolution of the dispersion
element. Examples of spectra collected with both the configurations will be shown in
the next pages. The multimode fibers allow the connectors and other optical
elements in the path, such as the laser injector, to be less critical in alignment [II.57].
In its last configuration, RRS takes advantage of the coupling by optical fibers to
switch to a laboratory version of the instrument which adopts a more traditional
layout. This transformation is achieved by connecting the laser source and the
detection apparatus to a fixed Raman probe, equipped with a interchangeable
microscope objective and mounted on a micrometric translator along the three
Cartesian axes. The converted instrument is adopted when, for laboratory analysis, a
more precise single-point analysis is needed: in this way, with an easy operation of
disconnecting and plugging two optical fibers, a second set-up is obtained.
II.6 RRS: the custom-made systems.
The optical system.
As shown in Fig. II.1, the design of the optical system stems from the requirement of
directing the parallel laser beam deflected by the 2-axis galvanometric scanner to
any point on the surface of interest. Hence, the X, Y coordinates in the area of
interest are mapped by the θ, ϕ angular positions of the galvanometric (galvo)
mirrors. Reversing the optical path, the Raman light collected by the optical system
64
is delivered to the galvo mirrors in a collimated beam and deflected towards the
detection unit. Since this task is definitely more critical than the handling of the laser
light, the analysis of the optical system described henceforth refers to the gathering
of the Raman scattering. Three main requirements have been critical in the design of
the optical system. The working distance of the Remote Raman Scanner should not
be shorter than 20 cm; this is the minimum value that grants a practical in situ
employment of the instrument. A safe non-contact working distance is preferable, as
previously mentioned, for the analysis of works of art. The second requirement
concerns the need for satisfactory mapping of heterogeneous paintings or
sculptures, and therefore the development of an instrument capable of analyzing
areas on the scale of tens of square centimeters. A flat field and absence of vignetting
over the whole field of view are also needed to achieve semi-quantitative Raman
measurements. A further issue that has challenged the design of the optical system is
the very low cross section of Raman scattering. This results in the need for as large a
numerical aperture as possible in order to maximize the collection of Raman signal.
To fulfill this requirement, a frontal lens with a 51-mm diameter has been chosen.
Considering a working distance for the optical system close to 20 cm, this leads to an
f-number (f/#) around 4. On the other hand, to limit the weight of the head of the
Raman spectrometer, the diameter of the scanning mirrors has been limited to about
10 mm. This means that the optical system must be able to direct as much Raman
light as possible from a large entrance pupil (51 mm) to a smaller exit pupil. A final
critical point is represented by aberrations: while chromatic aberration is virtually
negligible due to the narrow band of the Raman signal, spherical aberrations limit
the field of view of the optical system. After an in-depth study of the light path, a 4-
lens system was chosen as the simplest option for the construction of the device.
Specifically, a sequence of a positive lens, a negative lens, and finally two positive
lenses provided the desired properties of the light path. The adoption of a higher
number of lenses would provide a higher flexibility, but at the same time it would
increase the aberrations and the losses due to reflections. When considering a 4-lens
system, the values of the 4 focal lengths and those of the 3 distances between the
lenses are the parameters of the project, yielding a total of 7 degrees of freedom. In
addition, lens diameters and glass types could be used as additional parameters, but,
for the sake of simplicity, we decided to work with off the shelf (commercially
65
available) lenses, all having the same diameter of 51 mm. This choice reduces
assembling complexity and project costs.
After a preliminary project based on standard lens design criteria, the optimal
configuration of this system was optimized using the ray tracing software ZEMAX
(Development Corporation, USA). A virtual replica of the scanning device was
implemented for simulating the optical path. For the sake of simplicity, the ray
tracing was simulated only in a 2D space: this is a reasonable approximation, since
the optical system shows cylindrical symmetry. In addition, Zemax allows the
comparison between lenses of different manufacturers: the very same design has
been tested using lenses of seven brands. The simulations were addressed to
maximize a figure of merit that describes the Raman scattering power that crosses
the exit pupil of the optical system for each detection point on the surface of interest.
According to the simulations, Optosigma (USA) manufactures the elements that best
fit our specifications: the choice or this project was to adopt an aspheric lens of 50
mm focal length f.l. , followed by a divergent lens f.l. mm and a pair of
identical biconvex lenses (f.l. = 52.7 mm). The optimal distances between these
lenses were 20, 31, and 45 mm: the distance between the last lens and the galvo
mirrors is then determined by the position of the exit pupil, and is equal to 35 mm.
66
Fig. II.2. The quoted project of the optical system; distances between the lenses have been optimized
by Zemax.
Fig. II.3. Simulated collection efficiency ε r for the optical system as a function of the displacement of
the sample along the plane of the field of view, for a surface at a distance of 20 cm from the external
lens
67
The final project configuration is shown in Fig. II.2. If the theoretical beam path was
drawn, it would be possible to see that not all the collected light reaches the
scanning mirrors. In order to theoretically evaluate the capabilities of the designed
optical system, we simulated its collection efficiency ε r as a function of the radial
position on the surface of interest. ε r was estimated as the percentage of the
Raman light, scattered by the point on the sample surface at distance r from the
optical axis, which is able to cross the exit pupil. A Lambertian distribution was
assumed for the Raman radiant intensity. The result is shown in Fig. II.3: it is
possible to observe that the theoretical field of view is ∼12 cm in lateral size, and
that the collection efficiency is reasonably uniform within this area. It should be
further noted that the simulated collection efficiency is rather low (close to 0.3%).
Nevertheless, this value is close to the theoretical collection efficiency of an ideal
optical system with an f/# of 4 (approximately 1.5%). The lower efficiency of the
designed optical system is mainly ascribable to the smaller size of the footprint of
the scanning mirrors compared to the exit pupil. A better performance could be
achieved by increasing the mirror size, within the limits of loading allowance of the
galvo scanner; bigger deflection set-ups are available on the market, but they are not
tailored to this kind of employment and therefore they would represent a bulky and
unconfortable alternative for the overall probe dimensions and weight [II.54].
The software.
An user-friendly virtual interface was developed in order to manage all the devices
which can be controlled by the computer, and at the same time to monitor, acquire
and organize the collected data. The aim of the software, called RRS, is to provide to
the researcher an high-level access to the experimental parameters which he or she
reasonably needs to interact with, while hiding the most basic technical instruction
which must be given to the machines.
The software was programmed in the C++ language, and the code has been written
and compiled with the help of the LabWindows® suite (National Instrument, USA).
The control of the several devices relies on the libraries furnished by the producers
of the CCD, spectrograph and galvanometric scanner (Andor, Acton Research and
Cambridge Technology respectively).
68
In its current version (2.0), it is possible to manage the galvanometric mirrors, the
spectrograph and the CCD, while the parameters belonging to the laser source
(emission wavelength, exit power) can be inserted manually: in the next release, the
laser will be controlled by software, as well. It is planned, as well, to connect a
webcam to the probe head, and to show the image of the target area in a inset of the
interface window.
Taking inspiration from the most common commercial software, the program menu
offers a variety of options, which range from three operating procedures to the
instrumental settings to the usual file managing commands. What is unique in RRS
with respect to similar applications, is the possibility to set different points of
analysis and watch the system automatically deflecting the laser focus on the
selected position and starting the measurement. The possible working regimes are
three: the Run mode is used to monitor the evolution of the signal in real time,
without any average operation; Acquire is used for a standard measurement where
the laser spot position is fixed; Scan, instead, performs the analysis on the set of
selected points, acquiring and showing a spectrum per each position of the focus.
The file menu, in the end, allows the loading and the saving operations for one
spectrum or a set of spectra.
The graphic interface of RRS is shown in picture II.4: the main commands which can
be given to the instrument are distributed according to the system they refer to. The
selection of the laser focus position inside the field of view and the definition of the
pattern of the various analysis positions are some of the available operations in the
Mirrors sub-menu. The Spectrograph bar, instead, allows the user to choose the
diffraction grating and to position it to a specific central wavelength position. The
CCD menu is the most complex. A window for the temperature control of the
charged coupled device opens automatically when the software is started, and can
be accessed at any moment between the acquisitions, to set the cooling options. The
Region of Interest (ROI) of the silicon chip in which the analysis must be performed
can be defined via a dedicated window, as well as the vertical binning, if the sensor
is acquiring in imaging mode. The default operations, however, occur in
spectroscopy mode: this option enables a full vertical binning of the pixels, so that
the main window shows the intensity profile of the captured light, which, if properly
calibrated along the horizontal axis, corresponds to the spectrum. With regard to
69
this aspect of the measurement, a preliminary operation to each working session is
the acquisition or the loading of a reference spectrum, which ensures the correct
correspondence between the horizontal pixels and the chosen spectral coordinate
(frequency, wavelength, wavenumber, relative wavenumber): this task can be easily
accomplished via a dedicated panel. The last important parameters to be submitted
to the program are the exposure times for the acquisitions. Again, three possibilities
are given to the user, according to the working regime. The researcher can decide to
set a fixed exposure time, which will be applied to the single or to all the points of
analysis; otherwise, different exposure times, set by the user, can be applied to each
position of the laser spot; finally, an automatic procedure can be started, which
regulates the exposure time in order to achieve the selected signal intensity. This
functionality employs a trial-and-error method, in which the software guesses the
correct exposure time, tests it and then evaluates if the chosen value satisfied or not
the required signal to noise ratio: in this way, RRS automatically moves towards an
optimal exposure time; however, to prevent an exceedingly long process in
particularly unfortunate cases, a maximum number of repetitions can be entered. It
is worth to stress that, beside the exposure time of the single acquisition, a number
of accumulations can be planned per each spectrum: this method performs a
summation of the collected spectra of the same point of analysis to reduce the
statistically random contribution of the shot noise to the signal.
RRS software exhibits a communication window in its upper part, to provide the
user confirm of each inserted parameter, and to report the successful or not
execution of the given commands. The set of experimental parameters, furthermore,
are saved in the header of each spectrum file (bearing the e tension “.rrs” and can
thus be recovered together with the acquired data.
70
Fig. II.4. the graphic interface of RRS software in a typical Raman measurement. The yellow led on the
left top of the window indicates that a Scan measurement is running, and the coloured bar in the
lower part of the interface shows the progress of the acquisition.
71
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77
CHAPTER III.
RRS AT WORK: TESTS AND CASE STUDIES.
The previous chapter introduced the Remote Raman Scanner by explaining the
driving concept behind its development. This chapter reports the several tests which
have been performed to evaluate its behavior with respect to the planned
characteristic: the instrument performances have been assessed through
experiments with known samples. After a positive validation, the device has been
used for a series of analysis, on a heterogeneous set of samples, both as a punctual
source of information and as a mapping technique. Unfortunately, no chance to
employ the device in situ occurred until now; yet, the set-up was adopted for the
reported measurements in its ultimate configuration, and therefore ready to be
transferred without altering its structure; moreover, the long working distance
proved to be a useful property also for laboratory analysis.
III.1 Characterization of the performances.
Ad hoc tests have been performed to assess the depth and the flatness of the field of
view, the spatial resolution and the spectral accuracy of the developed system. A
series of other tests have been carried out on standard samples of several pigments
and binding media in order to appreciate the effectiveness of the device with
different materials and to evaluate the typical signal to noise ratio which can be
achieved for this kind of analysis; the spectra, not provided here, were collected in a
little database, in order to be used as references for comparison.
78
Assessment of the depth of the field of view.
The first test aims to the determination of the dependence of the collected Raman
signal on the displacement of the target object along the optical axis (z). For the
purpose, a Cinnabar (HgS) reference was placed in front of the Remote Raman
Scanner and moved along the z axis within the distance range 18.5-24 cm with a step
size of half centimeter. A Raman spectrum was collected per each position, with an
acquisition time of 10 s and a power density on the sample of 300 W/cm2;
successively, the intensity of the main Raman band of HgS, correspondent to Hg-S
symmetric stretching, (νs = 252 cm-1 [III.1]) was plotted with respect to the z-axis
position. The resulting curve is shown in fig. III.1. It is possible to notice how the
system provides a smooth variation in the collection efficiency in the selected range:
an estimation of the depth of field is given by the full-width half maximum (FWHM)
of the curve, approximately equal to 60 mm. The maximum efficiency occurs at a
working distance of 20.5 cm, a value which is in good agreement with the project
specification for the focal length.
Fig. III.1. Intensity curve of the 252 cm-1 Raman band of HgS, collected at different positions of the
target sample along the optical axis.
79
Assessment of the field of view.
The dependence of the collection efficiency on the focal plane has been evaluated as
well. A ColorChecker White Balance Card (X-rite, USA) is a board 20.9 x 27.9 cm2
wide covered with a uniform Titanium white (TiO2) layer, typically used for
checking the light uniformity of the field of view [III.2]; here it was employed as a
spatially uniform sample, and placed at the optimal distance from the most external
lens of the Raman scanning device (20.5 cm). A double line-scan was performed on
the two perpendicular axes (x and y) which cross the optical axis. The whole range
permitted by the mirrors deflection (± 4 cm in both directions) has been explored,
with a step size of 0.5 cm; the employed laser power density on the sample was of
300 w/cm2, while the acquisition time was of 20 s per each point. The intensity of
the reference Raman band of Titanium white, corresponding to the Ti-O symmetric
stretching (442 cm-1) was extracted from each spectrum, and after baseline
correction, it was recorded. The plot of the two curves obtained along the x and y
axes can be seen in figure III.2. Despite being both curves slightly asymmetrical, it is
possible to appreciate that within the interval -30 mm, +25 mm along both axes,
choosing the optical axis as the origin of the frame of reference) the collected
intensity is fairly flat. An estimate of the width of the possibly analyzed area, by
considering again the FWHM, is about 65 mm for both directions: for higher angular
deflections, the collection efficiency decreases quite drastically.
This area is smaller by a factor of 1.5 with respect to the simulated one. This
overestimation is mainly due to the fact that the virtual replica of the galvo mirrors
can freely rotate, while the VM1000+ scanning mirrors have a limited angular range
(±40°); the laser beam, therefore, can be deflected within a solid angle which is
contained within the aperture of the optical system, but that does not fill it
completely.
80
Fig. II.2. Intensity profile of the 442 cm-1 Raman band of TiO2 as collected from different points of the
target surface perpendicular the optical axis, along the horizontal (x) and vertical (y) coordinates.
Assessment of the spectral accuracy.
The spectra obtained by the latter measurements were also exploited to evaluate the
spectral accuracy of the Remote Raman Scanner. In other words, the shift on the
wavenumber axis undergone by the vibrational band at 442 cm-1, taken as a
reference, was measured for each focus position. This shift is actually an artifact due
to slightly different coupling of the backscattering light with the optical fiber which
“feeds” the spectrograph: its highest value was equal to cm-1, a result which is of
the same order of magnitude of the spectral resolution of the instrument, and much
lower than the FWHM of the TiO2 Raman band (19 cm-1). It is hence evident that the
uncertainty of the spectral coordinate in the Raman spectrum is negligible with
respect to the resolution of the spectrograph.
Assessment of the spatial resolution.
For the applications of purpose, the Remote Raman scanning does not need
extremely high spatial resolution: variations of the vibrational signal on micrometric
distances are more suitably revealed by a Raman microscope. Theoretically
81
however, the granularity of the galvo mirrors allows a precision of the order of 4 µm
(80mm of lateral width/ 20000 angular steps) in the focus positioning. On the
contrary, the laser spot size is approximately 200 µm wide because of the particular
choice on the employed optical system, and in order to maintain a low risk of
damaging the target sample with an high power density. However, it is necessary to
provide at least an indication of the spatial resolution, in order to estimate the
uncertainty at which the position of the analyzed point can be determined.
The spatial resolution of the scanning device was derived by the measurement of the
Edge Response Function (ERF). This is the intensity curve obtained when observing
an ideal step profile and it is strictly related to the spatial resolution of the device. In
fact, this quantity can be estimated through the so-called “rise distance” of the RF,
i.e., the distance for the signal intensity to change from 10% to 90% in
correspondence of the edge. The same definition can be adopted to indicate the
reversed distance (90%–10%) in the falling edge.
In order to assess this feature, a reference sample was created by making two
grooves with a width of 800 μm, separated by a distance of 10.5 mm, on a flat
aluminum surface. Each groove was filled with Titanium white (powdered Rutile).
The spatial transition from metal (no signal) to the synthetic mineral (Raman
signal) can be considered as an ideal edge. The sample was scanned along a line
perpendicular to the two white stripes with a variable step size equal to 70 μm in
correspondence of the edges and to 300 μm in the region between the stripes. It
should be noted that the intensity profile (fig. ZZ) of the two grooves is slightly
asymmetric, since the falling edges are steeper than the rising one: this must be
assigned to a non-perfect alignment of the sample with the field of view.
Nonetheless, if the average value is taken of the the “upwards” and “downwards”
edges, the result does not lose its significance.
The mean “rise distance” as defined above of the intensity of the Raman signal of
TiO2 by considering both of the two white stripes was estimated as 430 ± 130 μm
(Fig. 6). It can be inferred that the spot size of the focused laser beam does not
represent a limiting factor for the resolution of the device.
82
Fig. III.2. Intensity profile of the 443 cm-1 Raman band of TiO2 contained in two 800 µm-wide grooves
(whose position is shown in gray) on a metal surface.
III.2 A multi-analytical approach to a model painting.
The set-up has been used to record spectral information from a model panel
painting naturally aged in ambient conditions for 25 years. The model was prepared
by prof. Aviva Burnstock of Courtald Institute of Art, London, using traditional
pigments from a local supplier including lead white, gypsum, ultramarine (a sodium
aluminium silicate), and vermillion (HgS) bound in an egg-based binding medium
(Fig. III.4) [III.3]. The panel is divided into two smaller paintings, both of which have
been interested by the different studies. The left one is characterized by an area
covered by a gilding; the latter will not be covered by Raman spectroscopy
measurements. Two other techniques, among the most common for this kind of
studies, have been employed: reflectance multispectral imaging and X-ray
Fluorescence.
The necessity to use more than one analytical technique for a single identification
and diagnosis set of measurements is indeed well known [III.4]. For this reason,
several mobile instruments are employed together at the measurement site [III.5,
83
III.6] or, alternatively, multipurpose devices are being developed [III.7]. The purpose
of this laboratory test is to reproduce, in little, a in situ analysis of a work of art, and,
in particular, to validate the results supplied by the Remote Raman spectrometer
with data coming from complementary methods.
Fig. III.4. Model panel used to test the ability of the Remote Raman Scanner to identify pigments. The
materials and techniques employed for its realization are faithful to traditional egg-based painting.
Reflectance spectra and reconstructed maps.
The reflectance multispectral (rMI) imaging unit is a portable instrument which
acquires a series of reflected images of the object of interest, each one in a narrow
spectral interval. The device consists of two voltage-stabilized 150 W tungsten
halogen lamps (DLH4, Dedotec, USA) placed approximately at an incident angle of
45° with respect to the normal of the painted surface. The radiation reflected from
the surface is acquired with a low noise CCD camera (Retiga2000, QImaging,
84
Canada) coupled to a band-pass liquid crystal tunable filter (Varispec, CRi, USA),
which is used to scan across the visible spectrum. The measurement protocol
involves the acquisition of 65 images, each one related to the light reflected by the
surface in a different spectral band from 400 to 720 nm in 5 nm steps. The non-
uniform illumination of the field of view is corrected with the aid of a white balance
paper (Gretag Macbeth ColorChecker White Balance, USA); for the estimation of the
reflectance factor ρx,y( ) in each point of the field of view, data calibration is
performed using a calibrated 99% diffuse reflectance standard (SphereOptics, USA)
[III.2].
Each measurement provides, thus, a set of 65 images (1200×1600 pixels); if the
intensity values of a single pixel in each image are collected in a 65-elements array,
the reflectance spectrum of the point corresponding to that pixel is obtained. This
means that the result of each measurement is multi-spectral cube, a 3d matrix
whose dimensions are the two spatial coordinates corresponding to the points of the
image, and the spectral coordinate which varies in the interval 400-720 nm.
The raw data cube, therefore, provides straightforward information when it is
sectioned by a plane parallel to one of its faces. However, in most cases a more
synthetic expression of the collected data is needed in order to proceed with a more
refined analysis. For example, areas of the painted surfaces characterized by
different spectral features are highlighted by applying a supervised classification
algorithm based on the similarity between a reference reflectance spectrum (chosen
in correspondence to a certain area in the field of view) and each reflectance
spectrum of the analyzed surface [III.8]. The approach based on the Spectral Angle
Mapper classification (SAM) has been followed, where both the reference spectrum
and the measured spectrum ρx,y( ) at location (x,y) are treated as vectors. The
spectral angle between them, calculated according to the following equation,
, arccos ,
,
is taken into account as the similarity index, small angle values suggesting a high
degree of similarity.
(III.1)
85
For the panel under investigation, four reference spectra, corresponding to the most
common distinguishable colors, have been selected (Fig. III.5). The first one,
indicated as data1, corresponds to a point in the dark blue shadow of the lady’s vest,
in the right picture; the second refers to the red color adopted for the semicircle
surrounded by the guilding, this in the left-hand part of the panel. The third selection
(data3) has been made on a pink area corresponding to the lady’s cheek; the fourth,
instead, is located on the pale skin of the lady’s face.
Fig. III.5. Reflectance spectra of the sampled points on the panel. Data1refers to the blue color in the
painting, data2 to the red, data3 to the pink and data4 to the white.
Similarity maps were reconstructed for each of the selected spectra: in figure III.6
they are listed according to the chosen order. Each pixel is colored on a gray scale,
according to the value of the spectral angle between the reference spectrum and the
spectrum of that point: white indicates a null angle and therefore perfect similarity,
black the opposite.
86
Fig. III.6. Similarity maps of the painted panel, obtained with the selected reference spectra. From top
to bottom, left to right: similarity map for the blue (data1), red (data2), pink (data3) and white
(data4) color respectively.
The similarity maps conveys an immediate description of the distribution of the area
with analogous reflectance spectrum; this representation provides a much more
powerful information than a single reflectance map, revealing the spatial
distribution not of a single spectral band, but of a set of spectra. In the case of
interest, the panel painting results clearly segmented into four images which can
almost be superimposed without overlaying. Even though in this case study the
selected colors are significantly different, the adopted method is able to reveal
spectral similarities also in less distinguishable situations [III.2].
Despite the fact that reflectance imaging alone cannot, unless very favorable cases
[III.9], reveal the identity of a pigment, it is clear how it can significantly simplify the
role of subsequent analytical methods: in this case, the identification of the pigments
can be limited to four points of the studied area, without losing in the generality of
the collected information.
87
XRF analysis.
X-rays are electromagnetic waves emitted during highly energetic electronic
transitions within the atoms provoked by the bombardment of a target with charged
particles (electrons or ions) or with high energy radiation. They can be used for
obtaining transmission images of the works of art (radiography) or as a
spectroscopy source. In the second case, a detector is used to collect the
fluorescence photons emitted after X-ray interacting with the target material. Since
this high-energy fluorescence is related to the atomic energy structure, X-Ray
fluorescence (XRF) is a fast spectroscopic technique to provide the identification
and, possibly, quantification of the atoms contained into the object of interest. Being
the X-ray penetration depth inversely proportional to the atomic mass, almost all the
elements having an atomic number above a certain threshold can be detected. In
portable detectors, especially useful for the analysis of cultural heritage, the lighter
detectable atom is usually sodium 11Na. The limit to detectable elements is given by
the presence of air and by the entrance window of the detector, which is usually
made of a low atomic number element (Beryllium).
In collaboration of XGLab, a spin-off company of Politecnico di Milano, a series of
Energy dispersed X-ray fluorescence (ED-XRF) punctual measurements have been
performed on the painted panel. For the analysis, the latest portable device, called
ELIO, was employed. Equipped with a large area Silicon drift detector (25 mm2), it
can work in high resolution or in fast mode according to the input photon energy. Its
excitation source is a transmission X-Ray generator consisting of an Rh anode; the
instrument is particularly suitable for the analysis of cultural heritage thanks to a
couple of pointing laser (one on the axial and one on the focal direction), and to a
microscope camera which monitors a 20×20 mm2 area around the analyzed point:
the working distance is of the order of few millimeters. With a weight of 2.1 kg, ELIO
is a truly portable instrument: for the sake of reproducibility and comfort, however,
it was not hand-held during the measurement, but lodged on a tripod.
Four points of analysis (plus one on the gilding) have been chosen on the panel
surface, according to the selection performed through reflectance imaging. The
measurements have been performed in acquisition times of about 40-60 s each, and
the emitting tube was supplied with a 40 kV voltage (20 µA of current). The
resulting spectra have been reported in figure III.7 the portable instrument
88
automatically provides an interpretation for the distinguished peaks.. The top one is
related to the blue areas: the main constituting element is sulfur, with a small
percentage of lead. The latter being related to lead white pigment (lead basic
carbonate, 2PbCO3·Pb(OH)2), the only responsible for the blue color should be
sulfur. Among the traditionally available pigments, only lazurite (a.k.a. Ultramarine
blue, Na8(Al6Si6O24)Sn, n = 2-3) contains sulfur: a safe identification, however, is not
possible on this sole evidence. Despite the fact that sulfur is also a common element
in many other pigments, in this case the high relative concentration of this element
(~97%) suggests that it cannot simply be present in the underlying layers, but it
must actually take place in the blue pigment on top. Fluorescence emission of the
red spot, again, reveals a two-elements composition. In this case, however, the
relative concentration is almost equal to unity for the first one, mercury, whereas
iron is limited to the 0.71%. Mercury sulfide (HgS), as previously stated, can be
found naturally as cinnabar: from antiquity this mineral has been used as a pigment
and it is called vermilion. The iron oxide Fe2O3 constitutes another historical (and
archaeological) red pigment, red ochre. Its presence could be considered because
the statistical confidence interval, associated with the measurement, is quite high:
however, the low statistical uncertainty related to Hg, and the bright red color of the
selected area support the identification of the red pigment with vermilion.
XRF spectrum of the lady’s cheek, selected as the reference area for the pink color,
reveals the presence of lead, mercury and iron. This suggests a reasonable synthesis
of the pink color as a mix of lead white, vermilion and possibly red ochre: the iron
component (3%) in the fluorescence spectra is, indeed, not negligible in this case,
and red ochre could be used to provide a more realistic color to the skin. This
suggestion is confirmed by the spectrum of the white selected area, corresponding
to the lady’s nose and forehead. In this case, only lead and iron can be traced:
however, the relative composition of lead is increased, coherently with the
hypothesis of a mix of lead white and red ochre. No evidence of vermilion is here
found, and this is in agreement with the different reflectance spectra obtained for
the cheeks and the rest of the face.
Two more analysis have been performed out of the four reference areas, and
involved the white background of the two figures and the gilding. The first is rather
uniform throughout the panel, and thus a single acquisition was carried out. It
89
needed quite a long exposure time (180 s) to obtain the spectrum reported in the
higher part of figure III.7bis. The reason is justified by the table of the composition:
the two detected elements are rather light, and they are sulfur (~53%) and calcium
(~47%). The presence of this two elements in grossly equal percentages, hints at
gypsum (Calcium sulfate, CaSO4) as the ground layer which was likely used by the
artist.
The gilding was not expected to be real gold, still XRF reveals a non-negligible
(>13%) composition of this metal, the rest being mainly iron. Another significant
result is the detection of calcium, which at approximately 11% of the total
composition is the third detected element: not visible to the naked eye, this calcium
must probably be assigned to the gypsum used as the adhesive to fix the gilding to
the panel, according to one of the traditional methods for these decorations.
Sample name Element Concentration (%) Estimated error (%)
Blue S
Pb
96.94
2.8
2.20
0.99
Red Hg
Fe
99.29
0.71
0.64
5.63
Pink Pb
Hg
Fe
90.57
6.38
3.05
0.74
2.13
3.08
White Pb
Fe
98.77
1.23
0.56
6.54
Gilding Fe
Au
Ca
As
74.08
13.26
10.79
0.72
0.49
1.63
3.91
4.36
Tab. III.1. Elements detected by XRF in the selected areas of the panel.
Fig. III.7 (next page). XRF spectra of the four selected areas, from top to bottom: blue, red, pink and
white.
90
91
Fig. III.7 bis. XRF spectra of the white background (top) and of the gilding layer (bottom).
Flexible Raman mapping.
With the comfort of the results of the first two techniques, selective Raman mapping
was used to obtain a molecular analysis of pigments in the different colors over the
surface. No need for a raster scanning was here recognized, so the laser beam has
been focused only on few positions within the field of view of the instrument. The
measurements were performed at a distance of 20 cm from the panel, with a laser
power density of 200 W/cm2 on the sample and an acquisition time of 50 s for each
analyzed point (20 for the red area). It is important to underline that during these
inspections the painting was not moved.
The first test allowed the identification of ultramarine as the blue pigment: the
spectrum (figure III.8a), indeed, reveals the 548 cm-1 band of the lazurite pigment,
due to the symmetric stretching of the S- ion [III.1]; the 1007 cm-1 band of gypsum is
also present, hinting that the hue of the color was dimmed with the white pigment,
92
or, more likely, that the blue color does not fully cover the underlying gypsum
preparation layer. The identification of this pigment, thus, could only be confirmed
by a molecular-sensitive technique such as Raman spectroscopy, because in this case
the information provided by XRF are not sufficient (the element composing
ultramarine blue, N, Al, Si, O and, to some extent, S, are indeed too light to be
effectively revealed by that technique). No fingerprints of lead white was detected in
this area, but the Raman cross-section of this Lead compound is not particularly big
at 785 nm and its presence is probably hidden by the background noise.
The spectrum of the red pigment is not provided here because it is not very different
from the one obtained by the pink area, reported in figure III.8b: indeed, the Raman
fingerprints of Vermilion are very intense (282, 343 cm-1). The difference between
the spectrum of the pure red and the pink selected points is the presence of the 1050
cm-1 band of lead white in the latter. The results are in good agreement with the XRF
analysis, even if it was not possible to distinguish any of the spectral fingerprints of
red ochre, which is probably under the limit of detection of our instrument.
The spectrum of the white part of the lady’s face fig. III.8c shows two close little
bands, the first one at 1007 cm-1 must be assigned to gypsum, whereas the second,
at 1050 cm-1, reveals the presence of lead white. Again there is no trace of iron oxide,
but this is coherent with the Raman spectrum of the pink areas.
The last spectrum of figure III.8 refers to the white background of the panel, and it
indeed reveals all the spectral fingerprints of CaSO4 in the selected spectral window:
420 cm-1 and 494 cm-1 are related to the molecule’s out of plane bending, whereas
620 cm-1 and 674 cm-1 to the in plane bending. The intense band at 1007 cm-1,
instead, is assigned to the symmetric stretching while 1132 cm-1 to the asymmestric
stretching of the sulfate ion in CaSO4 [III.10].
93
Fig. III.8. Raman spectra of three of the selected areas, and (at the bottom) the spectrum of the white
background.
94
III.3 Identification of white and fluorescent pigments.
In , a Fluorescence lifetime imaging FLIM analysis on the an Gogh’s
watercolor “Les bretonnes et le pardon de pont ven” e posed at the Galleria d’ rte
Moderna in Milan, revealed an uncommon luminescence arising from some of the
white-colored areas in the painting [III.11]. Our research group is currently trying to
determine the substance which is responsible for this behavior: before a more
extensive study can be performed directly on the artwork, a series of original early-
XX-century white pigments and contemporary luminescent pigments have been
gathered and analyzed with different techniques. Some of the data which have been
supplied by FLIM and multispectral fluorescence analysis strongly suggest
Lithopone (∼60% ZnS and ∼40% BaSO4) is the pigment used by Van Gogh for the, of
course unintentional, luminescent areas. Another hypothesis, though, is that an
unusually doped zinc oxide (ZnO) has been used as the white pigment. Normally,
these two pigments do not exhibit a long-lasting fluorescence like the one present on
the watercolor, still the presence of an accidental doping agent within the
compound, caused by a non-refined synthesis, may have reasonably caused the
pigment to be luminescent.
Along with other non-destructive methods, thus, Raman spectroscopy was used to
characterize samples in powder of Lithopone “Chamot” reference collection
pigments. In figure III.9, the Raman spectrum of the pigment produced by ACME in
1922 is compared to the spectrum of a standard Barium sulfate powder. It is
possible to identify the original pigment as Lithopone because of the small band
arising at 340 cm-1, characteristic of ZnS and not present in the spectrum of BaSO4.
The distinction of this vibrational fingerprint, therefore, would be the main target of
a Raman study of the actual watercolor: still, not all the selected Lithopone pigments
provided a sufficiently resolved spectrum to detect it clearly.
95
Fig. III.9. Raman spectrum of the sample of XX-century Lithopone (black) vs the Raman spectrum of
the Barium white standard (gray). The exposure time was 30 s, 5 accumulations are used, laser
power density is 200 W/cm2.
In order to have a reference on the currently available luminescent pigments, two
other samples included the commercially available Fluoreszenz Grün, a white glow-
in-the-dark pigment, and Nach-Leucht-Pigment Grün, a greenish white pigment,
bought by Kremer® Pigmente GmbH (Germany). These materials have been used to
characterize the fluorescence produced by expressly luminescent materials,
obtained by highly-doped semiconductors, with possible emission resulting by
casual doping of traditional pigments. No identification of the substances within the
commercial pigments was supplied by the producing company. The Raman analysis,
however, was able to recognize at least the most important compound within each
pigment. Fluoreszenz Grün, indeed, apparently contains Zn2SiO4, since the bands at
390, 890, 904 and 944 cm-1 can be easily detected [III.12]. Pigment Grün, instead,
showed Raman bands at 218, 348, 416, 608, 634 and 667 cm-1 which can be
assigned to zinc sulfide (ZnS) [III.12]. ZnS, indeed, is the most used phosphor in
cathode screens, but its luminescence property is activated by doping with acceptor
materials, like copper. Being one of the two compounds present in Lithopone, zinc
sulfide is likely to be the responsible of the luminescent behavior of the an Gogh’s
96
watercolor. The presence of a doping agent, however, cannot be easily revealed by
Raman spectroscopy: a X-Ray Fluorescence analysis would be, in this case, more
significant.
Fig. III.10. Raman spectrum of the sample of Zinc Sulfate (black) versus the spectrum of Pigment
Gruen. No baseline subtraction has been applied to the spectra, whose intensities have been
normalized.
Fig. III.11. Raman spectrum of the sample of Fluoreszenz Gruen compared with the of standard Zinc
Silicate. The spectra have been normalized but not baseline subtracted.
97
It is worth to stress that none of the reported spectra undergone baseline
subtraction; despite being strongly luminescent, they did not exhibit a significant
background when excited with the 785 nm laser.
III.4 Analysis of samples from the “Memoriale italiano” of
Auschwitz.
In 1980, the Italian National Association of the Former Deportee (ANED),
inaugurated a memorial inside the 21 block of the concentration camp in Auschwitz.
The monument is made of a painted spiral which winds throughout the barrack
guiding the visitor inside the building (fig. III.12); Pupino Samonà, inspired by a text
of Primo Levi, realized the 23 stripes which compose the spiral. The object of
interest is an aerograph painting on textiles and it is under the supervision of
Accademia di Brera. Considering a restoration, the personnel of the Accademia is
currently collecting samples to be examined with different spectroscopy methods,
such as Infrared and Raman spectroscopy. Some of these samples, catalogued with
an abbreviation citing the number of the object and the stripe of provenience, have
been studied by the Remote Raman Scanner, thanks to a collaboration with
Emanuela Nolfo, a PhD student of the Accademia.
Some of the collected spectra are reported here. P6A1 is a white fragment of the first
stripe, and indeed it contains spectral fingerprints of white pigments, namely
titanium white (TiO2, in its rutile form) and calcium carbonate (CaCO3). The
reported spectra was collected in .. seconds with the 600 grooves/mm grating. P4A2
refers to a Red fragment, in which, however, the bands of TiO2(248, 442, 610 cm-1)
and CaCO3 (711 e 1088 cm-1) are dominant over any evidence of a red pigment or
dye. P5E23 refers to a yellow fragment: the grating has been rotated in order to
extract the spectral information from another window. The spectrum allowed the
identification with the arylide monoazo-dye based pigment Yellow 1, a.k.a Hansa
yellow [III.13]. Its recognizable bands are 997, 1137, 1215, 1254, 1310, 1390, 1455,
1487, 1532, 1567, 1599, 1622, 1670 cm-1. Thanks to the partial superposition of this
and the former spectral range, the 1087 cm-1 of Calcium carbonate can be detected
in this spectrum as well.
98
Fig. III.12. a. Plant of the Italian memorial of Auschwitz, hosted in one of the original barracks
of the prison camp. b. A picture of the of the painted spirals in the third room.
a
b
99
Fig. III.13. Raman spectra of some of the samples e tracted by Samonà’s work in the Italian memorial
of Auschwitz. Exposure time: 50 s. Laser density power: 100 W/cm2. No correction applied.
100
Subsequent analysis with a Fourier-Transform Infrared absorption (FT-IR)
spectrometer revealed the presence of a vinyl material within each sample, evidence
of the glue used as a binding medium; on a particular sample. P6A1, it was possible
to distinguish the spectral fingerprints of the fiber. They matched quite well the IR
absorption bands of cellulose, which reveal that the stripes have been made of
cotton. The presence of this organic material, together with the vinyl glue, is
probably responsible for the significant background present in the reported spectra,
which does not prevent, however, the identification of the most significant Raman
bands.
III.5 Study of a 3D plastic object
Polymeric materials have been used extensively in the production of design objects
thanks to the versatility of their mechanical, physical and optical properties, which
have been finely tuned through the addition of various plasticizers, stabilizers,
colorants, and blends of different polymers: the heterogeneity and sensitivity of
polymeric materials make the conservation and analyses of design objects
particularly challenging [III.14].
In this application, for the first time the Remote Raman Scanner has been adopted to
study a non-flat surface. The object of interests are polymeric design products of the
1950s-1960s; among them, it is worth to mention one of Castiglioni’s lamps,
Taraxacum. The reported spectra, though refer to the well-known Grillo telephone,
designed in 1965 by Marco Zanuso and Richard Sapper and manufactured in Italy by
Siemens. Being revolutionary in its shape and in its practicality, the phone can be
seen in museums of modern art such as the Centre Pompidou in Paris, or the MoMA
in New York City. The sample described here is part of the collection of the Triennale
Exhibition in Milan: it has been studied as part of the PhD thesis of Francesca Toja
on the conservation of polymeric materials [III.14]. The Grillo here concerned is
excellently preserved, though at a fluorescence multispectral analysis it provided
quite a different response for the microphone and the rest of the handset: fig. III.14b
101
synthetically reports the difference in the reconstructed RGB coordinates which
correspond to a slight variation in the maximum of the fluorescence spectrum.
The Raman analysis was performed, then, to try to ascribe this difference in the
fluorescence properties to a possible modification of the composing polymer, due to
a variation in the light exposure of the two sides. The Grillo phone, thus, has been
placed in front of the instrument and opened so that both the two areas could be
reached by the laser focus without moving the sample. The two spectra, together
with the reference spectrum [III.15] of the constituting polymer (Acrylonite
Butadiene Styrene – ABS), are provided in figure III.15.
As it can be noticed, no apparent evidence of photo-induced degradation of the
surface is provided by the Raman spectra. Probably, the variation occurred only to
the very e ternal layer of the handset, or the instrument’s resolution does not allow
a sufficient sensitivity to determine if the detected bands underwent a shift.
However, it should be stressed that the instrument did not fail in the identification of
the plastic compound, with a remote acquisition of 20s exposure time and 180
W/cm2 laser density power in order not to damage the telephone with an excessive
dose of photons.
Fig. III.14. A picture of the Grillo in its open and close configuration, on the left. The reconstructed
RGB fluorescence image of the upper, lower and lateral views of the telephone, on the right.
102
Fig. III.15. Raman spectra of the two selected areas of Grillo, compared to a reference spectrum of
ABS
III.6. Mapping of a rock sample.
The capability of working with non-flat surfaces makes the Remote Raman Scanner
particularly advantageous also in situations that are not strictly related to the
Cultural Heritage framework. Thanks to a collaboration with the geologist Sabrina
Moneta of the Statale University of Milan, a number of rock samples have been
studied: the case reported here is chosen to show once again the capability of the
instrument to perform a flexible Raman scan of the target surface. In this case,
however, the collected set of data has been processed by another self-made
software, in order to produce Raman spectral maps of the considered area. Called
RamanViewer, this program has been developed with Matlab® R2007B and it
103
provides a comfortable interface to manage the data acquired and saved by RRS.
Among its other features, what is relevant to this purpose is the possibility to
reconstruct spectral map of the scanned area for a single or for an interval of
vibrational shifts. The user can specify the starting and ending vibrational position
of a selected Raman band (for instance, 1077-1097 cm-1 for the 1077 cm-1 band of
Calcium carbonate) and the program plots the intensity of the selected spectral
interval for each analyzed area, taking into account its spatial coordinates. The
resulting image is virtually insensitive of the underlying background, since the
software exploits an algorithm that calculates the area comprised between the
spectrum and the line connecting the two extremes specified by the user. Thanks to
this calculation, a preliminary normalization of the spectra is not needed to obtain a
meaningful spectral map.
The selected rock, mainly made of argillite with vains of calcite mineral, is pictured
in figure III.16: the analysis covered an area of approximately 20×15 mm2 across
one of the calcite vains. The measurements were performed at a distance of 20 cm
with a laser power density of 500 W/cm2. Exposure time was set as a constant for all
the 24 points on which the laser has been focused, and it was equal to 40 s; no
baseline subtraction was applied to the spectra. Figure III.17 reports three spectral
maps which, despite the very thin sampling of the selected points, clearly permit to
distinguish the spatial profile of three vains. Indeed, they have been obtained by
reconstructing the intensity map of the spectral intervals 270-292 cm-1, 1075-
1100 cm-1 and 455-480 cm-1 respectively: the first and the latter being consistent
with the most notable spectral feature of CaCO3 (282 and 1087 cm-1,), whereas the
second refers to the SiO2 symmetric stretching at 469 cm-1. The reported spectrum
represents the point of coordinates (-4.52, 0.96): no baseline subtraction was
applied. For clarity, also the band of CaCO3 at 710 cm-1, not used for the map, has
been marked.
This application, while not particularly interesting from the point of view of the
analysed samples, is aimed once again to evaluate the mapping performance of the
Remote Raman scanner on a particularly irregular shape. Within a collaboration
project with the Grand Egyptian Museum of Gyza, a series of tests on fragments of an
Egyptian cartonnage and of a wall of an Egyptian city dating to the Roman period
(31 b. C., 313 A.D.), have started recently with promising results, since the coverage
104
of the cartonnage and the decorations of the wall are mainly made of inorganic
materials. The next step is, then, the Raman mapping of this two samples: the second
will probably provide the first occasion to test the Remote Raman Scanner in situ.
Fig. III.16. Photograph of the argillite + calcite sample. The red square shows the central area of the
RRS field of view. The red dots correspond to the positions from which the spectra have been
collected.
105
Fig. III.17. a. Spectrum of the area of coordinates -4.52,0.96 of the surface. b. Maps of the area under
the bands at 289, 470 and 1087 cm-1 respectively. It is worth to notice that, while belonging to the
spectrum of Calcium carbonate, the spatial distribution of the first and the last chosen band is not
completely overlapping; the spatial distribution of SiO2 (470 cm-1), instead, is concentrated in the
second row on the right.
a
b
106
Bibliography.
[III.1] D. Marano, I. M. Catalano, and A. Monno, Pigment Identification on “Pietà” of
Barletta, Example of Renaissance Apulian Sculpture: a Raman Microscopy Study,
Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy, 64 (2006),
1147–50;
[III.2] D. Comelli, A. Nevin, G. Valentini, I.Osticioli, E. Castellucci, L. Toniolo and
others, Insights into Masolino’s Wall Paintings in Castiglione Olona: dvanced
Reflectance and Fluorescence Imaging Analysis, Journal of Cultural Heritage, 12
(2011), 11–18;
[III.3] A. Brambilla et al., A remote Raman scanning spectrometer for in situ
measurements of works of art, RSI (2011);
[III.4] C. Fotakis, D. Anglos and V. Zafiropoulos, Lasers in the preservation of Cultural
Heritage: Principles and Applications, Taylor & Francis (2006);
[III.5] C. Miliani, F. Rosi, B. G. Brunetti and A. Sgamellotti, In Situ Noninvasive Study
of Artworks: The MOLAB Multitechnique Approach., Accounts of chemical research,
43 (2010), 728–38;
[III.6] T.D. Chaplin, R. J.H. Clark and M.Martinón-Torres, A Combined Raman
Microscopy, XRF and SEM–EDX Study of Three Valuable Objects – A Large Painted
Leather Screen and Two Illuminated Title Pages in 17th Century Books of
Ordinances of the Worshipful Company of Barbers, London, Journal of Molecular
Structure, 976 (2010), 350–359;
[III.7] I. Osticioli, N.F.C. Mendes, A. Nevin, A. Zoppi, C. Lofrumento, M. Becucci, E.M.
Castelluci, A New Compact Instrument for Raman, Laser-induced Breakdown, and
Laser-induced Fluorescence Spectroscopy of Works of Art and Their Constituent
Materials, Review of scientific instruments, 80 (2009), 076109
[III.8] A. Pelagotti, A. Del Mastio, A. De Rosa, A. Piva, Multispectral Imaging of
Paintings, IEEE signal processing magazine (2008) 27–36.
107
[III.9] M. Bacci, M. Picollo, G. Trumpy, M. Tsukada, D. Kunzelman, Non-invasive
identification of white pigments on 20-th century oil paintings by using fiber optic
reflectance spectroscopy, The American Institute for Conservation of Historic &
Artistic Works, 46 (2011), 27–37;
[III.10] .D. Chaplin, R. J.H. Clark, D. Jacobs, K. Jensen, and G. D Smith, The Gutenberg
Bibles: Analysis of the Illuminations and Inks Using Raman Spectroscopy, Analytical
chemistry, 77 (2005), 3611–22;
[III.11] D. Comelli, A. Nevin, A. Brambilla, I. Osticioli, G. Valentini, L. Toniolo, and
others, ‘n the iscovery of an Unusual Luminescent Pigment in an Gogh’s Painting
“Les Bretonnes t Le Pardon e Pont ven, Applied Physics A, (2011);
[III.12] RRUFF, database of Raman spectra online (www.rruff.info);
[III.13] N. Scherrer, S. Zumbuehl, F. Delavy, A. Fritsch, and R. Kuehnen, Synthetic
organic pigments of the th and st century relevant to artist’s paints: Raman
spectra reference collection. Spectrochimica acta. Part A, Molecular and
biomolecular spectroscopy 73, no. 3 (August 2009): 505-24;
[III.14] F. Toja, A. Nevin, D. Comelli, M. Levi, R. Cubeddu and L. Toniolo, Fluorescence
and Fourier Transform Infrared Spectroscopy for the analysis of iconic Italian design
lamps made of polymeric materials, Francesca Toja. Analytical & Bioanalytical
Chemistry, 399 (2011) 9, 2977-2986;
[III.15] Tsuchida, Akihiro, Hirofumi Kawazumi, Arikata Kazuyoshi, and Tuchida
Yasuo, ‘Identification of Shredded Plastics in Milliseconds Using Raman
Spectroscopy for Recycling’, 2009 IEEE Sensors, (2009), 1473–1476;
108
CHAPTER IV
SERS ANALYSIS OF AMINO ACIDS WITH A
PORTABLE INSTRUMENT.
A different application of a portable Raman instrument is here described. This
chapter is more concerned on the employed technique, which is Surface-Enhanced
Raman Spectroscopy, than on the instrumentation: the described experiments,
indeed, involve the adoption of a commercial portable instrument for the SER
analysis of liquid and solid samples of amino acids. No in situ (with the meaning of
“out of laboratory” S RS e periment is, to date, published: this work, despite
relying on laboratory tests, validates the effectiveness of SER analysis of simple
molecules performed with a portable spectrometer. The purpose of this study is to
determine the crucial parameters and the critical points of this kind of application,
in order to pave the way for a real on-site employment of this method on samples of
cultural or archaeological importance.
The work here reported is part of a collaboration program between Politecnico di
Milano and the FOundation for Research and Tecnology – Hellas (FORTH) in
Heraklion. The present text reports the results of a research period of five months at
the Institute of Electronic Structure and Laser (IESL-FORTH) of Heraklion, under the
supervision of professor Demetrios Anglos.
IV.1. The aim of the work.
As introduced before, this research is a contribution to a wider project which has the
objective the development of new portable instruments and techniques for the
analysis of organic residuals in archaeological finds. The identification of these
remains, often extensively affected by age and degradation, is possible through the
109
detection of organic molecules (e.g. amino acids, fatty acids) which act as bio-
markers specifically related to particular compounds. There are a number of
situations, however, like the screening of the presence of organic substances, the
growth of fungi or the incidence of contaminants on a valuable object or monument,
where chemical analysis must be performed directly on site, and almost immediately
[IV.1]. The use of this type of in situ analysis, which can provide meaningful results
in a reasonable time, is particularly critical for archaeologists, conservators and
scientist involved in such studies. In this work, simple organic molecules were
chosen to assess the performance of SERS analysis with a portable instrument.
Amino acids, the building blocks of proteins, are common analytes for SERS and
several approaches for enhancing the Raman signal of these molecules have been
developed: past research, though, exploited bench-top Raman microscopes. Here, a
portable Raman spectrometer is applied to liquid and dried samples of amino acids
and small peptides in aqueous solution; the contribution of silver or gold colloid to
recovery the Raman fingerprints, lost after reducing the concentration of the
analytes, is evaluated.
The purpose of this study is not the development of a highly specific detection tool
for one molecule, but the evaluation of the minimum requirements for the device
and for sample preparation in order to obtain diagnostically significant spectra. In
this perspective, no ad hoc procedure was exploited to maximize the Raman cross
section of a specific sample. Although some considerations about particular cases
are reported, this work should be considered within a framework of the study of
biological samples and within the context of archaeological residue analysis.
IV.2 SERS of amino acids.
Amino acids are organic molecules in which one amino group (-NH2) and one
carboxylic acid group (-COOH) are connected to a so-called side chain, another
group specific for each amino acid. These compounds are the building blocks of
peptides, and hence, of proteins: their presence is, therefore, widespread in all
samples of biological origin. For this reason, they have been among the first
molecules to be analyzed with Raman spectroscopy [IV.2]; however, only samples in
crystalline form can be revealed without significant effort, and therefore their
110
spectra can be a valid reference only to a certain extent. G. Zhu et al. showed that
Raman analysis of 18 amino acids in various concentrations (but always above
0.01 M) is nowadays possible with a bench-top micro-Raman device, but most of the
spectral fingerprints are lost in the passage from solid to solution (especially for the
aromatic amino acids) or are altered due to shifts and broadening of the bands
[IV.3].
In general, several analytical techniques are employed for the detection and analysis
of proteins: according to the applications, chemical decomposition techniques can be
employed (hydrolysis followed by separated by ion-exchange chromatography or
hydrophobic interaction chromatography), or mass spectrometry. In archeological
applications, however, reference must be addressed to other techniques which,
while being sensitive for these molecules, are most suitable for the analysis of
residues or traces of materials contained in ancient vessels or fragments of pottery.
Normally the identification of these remains relies on different laboratory
techniques, including Fourier-Transform Infrared spectroscopy (FTIR) and Gas
Chromatography-Mass Spectrometry (GC-MS) [IV.4, IV.5].
As a diagnostic tool, Surface Enhanced Raman Spectroscopy (SERS) is particularly
suited for the analysis of organic molecules present even in very low concentrations
[IV.6,IV.7]. Many studies on proteins and amino acids have been carried out,
revealing the presence of these analytes in solutions (as low as 10-6 M [IV.6]). The
need for micro-samples, together with the requirement for minimal sample
preparation are the drawbacks of typical SERS measurements, yet they are largely
compensated by the massive increase in the signal to noise ratio and hence
sensitivity provided by the use of a suitable nano-structured substrate. In addition
to signal enhancement, SERS has a fluorescence quenching effect, which is extremely
desirable for the analysis of biological samples, as those usually exhibit a high
fluorescence background in Raman spectra excited by visible laser radiation [IV.8].
Experiments exploiting different materials, such as silver colloids, synthesized
following several recipes, gold containing chromatographic beads, silver films or
silver-coated glass fibers via Tollen’s reaction are described in the literature. In
particular, however, most of the reported methods focus on the use of metal
electrodes whose surface is artificially roughened before they are inserted in a
suitable cell containing the molecules in solution [IV.9, IV.10]; Stewart and
111
Fredericks, however, used a silver electrode as a substrate but left amino acid
solutions to evaporate [IV.11]. In the analysis of amino acids as part of this work,
silver and gold colloids synthesized according to Lee and Meisel’s and Leopold and
Lendl’s methods are used, not only because of their simple and cheaper production
coupled to their very good performance with a wide range of laser wavelengths and
analyte molecules: the main reason behind this choice is to test the portable
instrument with one of the most practical substrates if a in situ operation is
foreseen: silver and gold nanoparticles, indeed, if stored in a dark and refrigerated
environment, do not need any particular care before being applied and can be used
without any significant efficiency loss up to one month after their synthesis [IV.7].
SER analysis of amino acids, in synthesis, can be a key passage in developing an
effective non-destructive diagnostic technique for archaeological remains. However,
its role in the Cultural heritage field would not be limited to this application, thanks
to its high sensitivity to the molecules and their behavior, even in small
concentrations. The mechanisms involved in the chemistry of painting can be
interpreted, for example, with time-resolved spectral SER analysis: for example, this
method allowed Cañamares et al., [IV.12] to monitor the binding process between
alizarin and ovalbumin, employed in egg tempera.
The promising results obtained in the application of SERS must be consistent with
those furnished by other techniques, and above all, face particular problems
regarding experimental reproducibility: it is known, indeed, that spectral distortions
can occur with SER spectra. A key problem for the analytical application of SERS, and
especially for the characterization of biological samples, is to attain reproducible
signals combined with a large enhancement factor. The reproducibility of SERS
spectra and the achieved enhancement depends on many experimental factors,
including nature and morphology of SERS substrates, geometry of the analyte-metal
interface, as well as the excitation wavelength [IV.6]. This work will try to evaluate,
as far as possible, which of these factors influences the measurement most.
Nonetheless, a more complete set of experiments, using a bench-top
instrumentation, is necessary for a thorough description of the SERS of amino acids
which is beyond the scopeof the current project. In order to test the portable Raman
device as a suitable instrument for in situ SERS, research was focused on the
applicability of the method to samples of increasing complexity.
112
IV.3 SERS with metal nanoparticles.
A wide variety of SER substrates has been developed and is currently under test.
Among the first to be introduced are gold and silver nanoparticles, and they are still
one of the favorite choices for many analyses. The main reason is that their synthesis
does not rely on particularly expensive or sophisticated techniques or apparatus,
but they can be obtained via a chemical process that exploits the reduction of salts
or acids containing these two elements. The most reliable and most well-known
methods for synthesis were published in the 1982 by Lee and Meisel [IV.13]; the
majority of SERS measurements is based on these substrates [IV.14- IV.17]. It is
convenient, indeed, to exploit the silver colloid as a preliminary test for SER
measurements on a wide variety of substrates, and then to resort to more specific
nano-structured materials in case the obtained sensitivity is not sufficient. On the
other hand, in spite of relatively simple preparation methods, the production of
reproducible colloids with the desired size and shape seems to be difficult, hence
limiting the reproducibility of the resulting SERS spectra [IV.6].
113
Fig. IV.1. a TEM image (a) of the silver colloids, and their absorption spectrum (b).
This method, or metal nanoparticles in general, has found several applications in the
analysis of Cultural heritage: it has been applied for the detection of proteins
revealing binding media, of inks and organic dyes. All these substances, indeed, give
rise to a significant fluorescence background which hampers the detection of the
Raman spectra. In most cases, the analysis using SERS has been carried out on
replicas of painted layers or inked paper; when the analysis of the actual object of
interest was needed, the measurements have been performed on microscopic
samples, removed by surgical blades [IV.18], or extracted by superimposing a
polymer bead loaded with a delicate acidic solution [IV.19] on a sample. However, in
one interesting case, it was possible to perform SERS directly on the object of
interest, a 16th-century Turkish carpet [IV.7]: in this case, metal colloid was the only
114
practical possibility to enhance the Raman signal of a selected area (a bunch of
textile fibers) without altering the target object or the instrument set-up.
In the current project, one of the silver colloids was prepared according to two of
Lee and Meisel’s procedures [I . 3]. Briefly, an aqueous solution of silver nitrate 8
mg of AgNO3 – Sigma Aldrich, USA) in 0.1 L of ultra-pure water (Millipore) was
heated to its boiling point and 2 mL of trisodium citrate aqueous solution
(Na3C6H5O7, 1% – Sigma Aldrich, USA) was added; the solution was kept boiling for
one hour: macroscopically, this colloid (Ag-LM) was characterized by a warm
grayish color. A second solution (Ag-HA) was obtained starting again from silver
nitrate (18 mg/l) in 0.1 L of ultra-pure water; 4.5 ml of NaOH (0.1 M) was mixed to
5 ml of Hydroxylamine –Hydrochloride (NH2OH ·HCl, 0.06 M) and then was added
dropwise to the aqueous solution of silver. The mixture was then stirred at room
temperature until milky grey color is obtained. This method has been introduced in
2003 by Leopold and Lendl [IV.20] and can be more effective for laser excitation in
the NIR. gold colloid u was prepared following again Lee and Meisel’s method
involving trisodium citrate as a reducing agent. The starting compound for the
reaction is chloroauric acid (HAuCl4): a solution 10-3 M is obtained by mixing 240 mg
of HAuCl4 with 0.1 L of ultra-pure water and brought to boiling. Then 50 ml of a 1%
v/v sodium citrate is added and the resulting solution is kept boiling for 1 hour. All
the solutions have been conserved in a dark and refrigerated environment (4 °C)
and they were always stirred before application. They have been used for one month
after the synthesis and in this period they demonstrated a good stability.
The formation of the nanoparticles was followed by monitoring the surface Plasmon
resonance band on a Perkin Elmer Lambda 950 UV-Vis absorption spectrometer
from 200-1000 nm: additionally, Transmission Electron Microscopy (TEM) was
carried out with a JEOL JEM-2100 Electron Microscope operated at 200kV, equipped
with a high resolution digital imaging CCD camera (model 782, ES500W
ErlangshenTM Gatan Inc, USA) to take images of the nanoparticles. In figure IV.1a it
is possible to observe the TEM image of a sample of the Ag-LM colloid, dried on a
glass microscope slide. The observed nanoparticles are roughly spherical, and their
diameter is of the order of 50 nm. In figure IV.1b, the absorbance spectrum is
reported: the Surface Plasmon Resonance is located at 431 nm, in good agreement
with the published spectra of the colloid [IV.13, IV.21].
115
IV.4 The portable instrument.
Analysis of solid amino-acids using Raman spectroscopy outside of the laboratory
environment has been reported recently by A. Culka et al. [IV.22]. In this work a
similar approach is taken, with the difference that well-established SER substrates,
i.e. silver and gold colloids are adopted in an effort to exploit a higher detection
sensitivity [IV.1].
A mobile Raman Spectrometer (HE 785, Horiba – Jobin Yvon, France) is employed:
as shown in Figure IV.2, it is based on a 785 nm semiconductor laser source coupled
by an optical fiber (ø = 50 microns, 5 meters long) to a compact probe head which
contains the necessary optics for sample excitation and signal collection. The
focusing lens can be chosen from a set of microscope objectives with different
magnifications: for the experiments considered here, a 20x (0.2 NA) and a 50x (0.4
NA) objectives were used. Collection of the Raman scattering signal is provided by
the same objective which delivers the backscattered light through an edge filter (OD
= 4, cutoff = 53 cm-1) to a second optical fiber (ø = 50 µm, 5 m long) which is
connected to a concave fixed grating (950 grooves/mm) spectrograph and a Peltier-
cooled CCD detector (Horiba Synapse). This setup performs measurements in the
range 50-3200 cm-1, with a spectral resolution of 4 cm-1. Light power on the sample
can be regulated from a maximum of 30 mW to a minimum of 0.3 mW. The
LabSpec® software package was used for spectra acquisition and data handling. A
VGA camera is seated inside the mobile probe head to monitor the area under the
field of view of the objective lens: when a mirror is inserted via a dedicated lever in
the light path, the instrument can be operated as an ordinary microscope. The whole
head (20×15×30 cm3, 8 kg) is mounted on a precision micrometer stage, able to
move it along X, Y, Z directions: together with the viewing camera, this allows
correct positioning and focusing of the probe. The size of the whole set-up is such
that it can be mounted on a mobile support (60×40×80 cm3 approximately,
considering the control computer).
This system was described by Westlake et al. [IV.23] and it has been recently used at
the Archaeological Museum of Heraklion for the analysis of pigments on a wall
painting. The same system, equipped with another laser source and normally used
116
for the analysis of ceramics, glasses and enamels in museum collections, already
demonstrated to be suitable for in situ analysis: micro-Raman spectroscopy, indeed,
was performed on rock art in South Africa [IV.24] with a HE532 micro-Raman
spectrometer by Horiba Scientific (Jobin – Yvon, France) under very uncomfortable
working conditions.
Fig. IV.2. The layout of HE785. The interior of the probe head is shown in the grey box, whereas the
laser source and the detection unit (light blue) are connected with optical fibers. The movable mirror
(M) which intercepts the laser beam (red) to enable the vision by the viewing camera is shown in its
two possible configurations; EF (standing for Edge filter) discriminate between the inelastic
scattering and the reflected component of the collected light.
IV.5 Tests and results.
The considered amino acids are L-Arginine (L-Arg, (NH2)2-C-NH-(CH2)3-CH-(COO-
NH2+)), L-Methionine (L-Met, CH3–S–CH2–CH2–CH–(COO-NH2+)) and L-
Phenylalanine (L-Phe, (C6H5–CH2–CH–(COO- NH2)+)); a more complex molecule was
represented by one tri-peptide, Glutathione (γ -L-glutamyl-L-cysteinylglycine). They
117
serve as model compounds referring to building blocks of proteinaceous materials
found in archaeological residues. Considering the evaluation of the proposed SERS
methodology and of the mobile instrument used, the choice of amino acids was
based on their structures. One of the amino acids has an aromatic side chain (L-Phe),
one contains sulfur (L-Met) while L-Arg has only a nitrogen rich side chain. The
selection of these amino acids was made for two complementary reasons: to explore
any favorable sensitivity arising from side chain chemistry and at the same time to
avoid possible over-estimation of the SERS effect (for example, the bonding between
sulfur and the silver nanoparticles), in agreement with criteria outlined by Sharma
et al. [IV.25].
The analyses reported below include:
- Raman spectra of the amino-acids in their crystalline form and in solutions
10-1 M;
- SER spectrum of L-Met in solution 10-3 M;
- SER spectra of the amino acid solutions dried on a layer of silver
nanoparticles;
- SER spectra of dried L-Met solutions starting with different pH values;
- SER spectrum of a dried mixture of L-Met and L-Phe;
- SER spectrum of a tri-peptide (Glutathione).
Raman spectra of amino acids.
The selected amino acids have been acquired from Sigma Aldrich (USA) in their
crystal phase. On these very samples a set of preliminary Raman measurements was
performed in order to determine the order of magnitude of the signal intensity
which can be revealed, in normal condition, with the portable apparatus. The
spectra of the three amino acids, L-Arg, L-Met and L-Phe are reported as figures IV.4
a, b and c respectively: in all cases, the objective of choice was the 20× and the light
power density on the sample was approximately 250 W/cm2. For all samples the
acquisition was performed in 10 accumulations of 20 s each.
118
Fig. IV.3. The molecular formula of the three amino acids of choice. From left to right: L-Arg, (NH2)2-
C-NH-(CH2)3-CH-(COO-NH2+); L-Met, CH3–S–CH2–CH2–CH–(COO-NH2
+), L-Phe, (C6H5–CH2–CH–(COO
NH2+-)
It is possible to notice a series of well defined bands for each spectrum: the
resolution supplied by the grating is not a limiting factor for the discrimination of
the spectral features. In general, most spectral features are all are contained in the
interval 300 – 1600 cm-1, but for L-Arginine and L-Methionine it is possible to
distinguish also the bands of CH2 stretching at 2920 cm-1 and, for L-Arg, CH3
stretching at 2870 cm-1. In the next paragraphs, however, attention will be focused
on the”fingerprint” spectral window -1800 cm-1, because the major detected
bands fall in this region..
The most significant detected Raman bands for the three amino acids with spectral
attributions are listed in tables IV.1, IV.2 and IV.3 for L-Arg, L-Met and L-Phe
respectively.
119
Fig. IV.4. Raman spectra of amino acids in powder. From top to botton: L-Arg, L-Met, L-Phe
120
In addition to Raman spectra of solid samples, spectra of the 10-1 M solutions of the
three amino acids have been collected; however, it was not possible to detect
significant spectral fingerprints with the reported instrument. Even exploiting a
highly sensitive laboratory Raman microscope (Nicolet Almega XR, Thermo
Scientific, USA), only L-Arginine and L-Methionine provided some recognizable band
structures. Despite the weakspectral features obtained by the portable instrument
HE785, an approximate quantitative assessment of the potential of the instrument
can be made. In figure IV.5 the signal obtained of L-Met in 50 s of acquisition at full
laser power is shown. The broad band arising between 1600 and 1700 cm-1, marked
by an asterisk, is due to the presence of water [IV.26]. Despite the very low quality of
the spectrum, it is possible to estimate the height of the Raman band at 1350 cm-1:
this intensity will be referred to the intensity of the correspondent SERS band to
obtain a rough estimate of the enhancement factor (EF) which can be obtained from
this measurement.
Fig. IV.5. Raman spectrum for 0.1 M L-Met. The asterisk marks the Raman band of liquid water
(symmetric stretching) at 1630 cm-1.
Analysis of liquid samples.
New solutions, obtained by gradual dilution of the 10-1 M of L-Arg, L-Met and L-Phe,
at intervals of 1:10 in volume, up to 10-6 M, were prepared. Three samples for each
of the three 10-3 M solutions were mixed in equal parts with Ag-LM, Ag-HA, Au
colloids respectively: in particular, a small volume (0.2 ml) of each mixture was
121
poured in a small, cylindrically shaped groove, machined on the surface of an
aluminum sample holder. Spectra have been collected 15 minutes after the solutions
were mixed; measurements have been performed by the 20× objective, the
maximum laser power (30 mW) on the sample and the average acquisition time was
50 s, with 10 accumulations per spectrum.
Since Ag-LM was the most effective colloid, every other sample solutions have been
mixed with this particular set of nanoparticles, with the same experimental
conditions (different parameters are explicitly reported). In general, however, the
quality of the SER spectra was not sufficient for the identification of the analyte. One
of the best results was obtained with L-Met (Fig. IV.6b). In contrast to normal Raman
spectra, the presence of Ag colloids in the amino acid solutions led to the
observation of several characteristic vibrational bands. It is possible to distinguish
several spectral features: 567 cm-1 (COO- wagging) [IV.22], 642 cm-1, 686 cm-1 (CS
symm. stretching), 770 cm-1 (CS stretching), 841 cm-1 (CC stretching), 925 cm-1, 950
cm-1 (CH3 rocking), 1031 cm-1 (CC stretching), 1181 cm-1 (CH stretching), 1363 cm-1
(CH3 symmetric stretching, COO- symmetric stretching) [IV.22], 1507 cm-1 (CN
asymm. stretching).
The Enhancement Factor (EF), defined in Maier [IV.27], with respect to a reference
solution prepared without Ag nanoparticles, cannot be calculated straightforwardly,
because of the absence of any visible Raman bands in the latter case. However, the
amplitude of the small band at 1350 cm-1 is observed in the Raman spectrum of the
10-1 M solution and was used to divide the height of the same band in the SER
spectrum: by taking into account the ratios between the concentrations and
between the exposure times, an indicative value for EF of approximately 2000 is
obtained. The spectrum is comparable to that reported by H. Lee et al. [6], if we
consider that the laser power is lower by a factor of 10 and the wavelength is further
from the nanoparticle plasmon resonance (785 vs 514 nm). With similar
considerations, the spectrum quality is similar to that acquired by Podstawka et al.
[IV.14] with a silver colloid synthesized by using NaBH4, even though they report a
larger number of bands.
The spectrum of 10-3 M L-Met was the most straightforward to acquire, with respect
to both the more and the less concentrated solutions of L-Met, which presented
distinguishable bands for concentrations as low as 10-5 M: it can be inferred that at
122
10-3 M the most effective coverage of the silver substrate is achieved for Methionine,
in agreement with Graff et al. [IV.9]. No unambiguous signal, however, could be
obtained from the L-Arg and L-Phe liquid samples. Therefore, further tests were
focused on dried samples of the same solutions: the concentration, from now on,
refers to the initial solution chosen as the sample, which though not strictly valid on
the solid sample, may be considered as indicative of the superficial density of the
adsorbed molecules.
Analysis of dried solutions.
Dried samples were also produced on a flat aluminum substrate, which does not
exhibit a significant background signal in the Raman spectrum. These samples are
not simply the dried version of the liquid mixtures, but a two-step procedure was
adopted to generate them. First a droplet (10 μl) of the silver colloid was placed on
the aluminum substrate and left to dry. The stain formed was covered with an equal
volume droplet of the amino-acid solution that was allowed to dry without heating.
This method is similar to the one described by Stewart et al. [IV.11] for the analysis
of amino acids on a roughened electrode; another comparable approach was
adopted by Huang et al. [IV.28], who heated the deposited colloid to remove the
solvent and aggregate the silver nanoparticles. Analysis was carried out with the
50× objective lens, and power density below 103 W/cm2 on the sample: integration
time, unless otherwise specified, was 10 s with 10 acquisitions per spectrum.
In figure IV.7, the SER spectra of L-Phe (10-4 M, a), L-Met (10-3 M, b) and L-Arg (10-4
M, c), deposited and dried over the evaporated colloid are shown; the main
detectable bands are labeled and assignments are reported in Tables 1, 2 and 3
respectively.
Following baseline subtraction the signal to noise ratio increases drastically with
respect to the liquid solution samples. This is particularly noticeable for spectra
acquired in pro imity of the “coffee ring” of the stain, where the density of the
deposited silver colloid is higher; the spectra are, nonetheless, representative of the
whole samples, and similar to typical spectral fingerprints found all over the surface.
The effectiveness of the metal layer produced by the evaporation of the colloid over
the substrate, together with the higher light collection provided by the 50× lens
with respect to the 20× on a relatively flat surface, combine to yield unambiguous
123
spectra for the three different amino acids, which are acquired in a time on the order
of one minute. Again, it is difficult to give an estimation of the EF because the Raman
spectrum of the same samples dried without the nanoparticle substrate does not
show any distinguishable features. Nonetheless, it is observed that the adopted
nanoparticles exhibit a preferential enhancement for bands in the spectral region
around 650, 1000 and 1300 cm-1. A comparison of the results obtained with L-Arg
and L-Met against other SER spectra recorded in similar works [IV.9, IV.29] indicates
that we detect a higher number of bands, whereas for L-Phe the quality of the
spectrum is similar to the one obtained by Lee et al. with silver nanoparticles and a
514.5 nm laser [IV.30].
Fig. IV.6. SER spectra of Methionine mixed with Silver colloid in liquid (b) and dried form (a). The
intensity scale of the b spectrum is multiplied by a factor of 40.
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Fig. IV.7 SER spectra of L-Phe (a), L-Met (b) and L-Arg (c) dried solutions (10s acquisition time, 10
scans, 104 mW/cm2 power density on the sample, 50x objective lens). The spectra are baseline
subtracted and normalised to maximum intensity for clarity.
Dependence of L-Met spectra on pH.
Amino acids in an aqueous solution may exist in three different forms, the anion, the
zwitterion or the cation, with the relative proportions determined by the isoelectric
point (pI) of the amino acid and the solution pH. The SER effect is known to be
strongly influenced by pH [IV.10, IV.28, IV.29]: with reference to the work of Graff et
al. [IV.9] and Abello et al. [IV.10], in this work the influence of pH variations on the
detection of SER signal was assessed only for L-Met. The pKa values of Methionine
are 3.3 for the carboxylic and 10.5 for the amino groups [IV.9], while the isoelectric
point is at 5.7: to monitor the evolution of the vibrational spectrum from the cationic
to the zwitterionic form, thus, a limited but significant range of pH values is
explored. The original solution of L-Met 10-3 M had a pH of 5.5, in agreement with
other references [IV.31]; two other 10-3 M solutions of Methionine in water were
prepared and adjusted to pH of 3.5 and 6.8 by adding HCl and NaOH respectively.
125
Since the quality of the spectra for the liquid samples does not allow many
considerations about the analytes in solution, it is necessary to follow the dry
approach also to monitor of the pH dependence. Dried samples obtained by the
standard 10-3 M L-Met solution, and two solutions at the same concentration with
adjusted pH values were analysed (with 20 s acquisition and 5 accumulations): the
results are shown in figure IV.8, where spectrum a refers to the cationic form (pH =
3.5) and c to the zwitterion (pH = 6.8). In both cases, the main distinguishable
bands, relative to C-S stretching for different rotamers, are located between 650 and
750 cm-1 [IV.31]: in this region some bands do not show significant shifts, but the
broad band at 662 (pH = 3.5) appears as a much narrower band and is shifted to
686 cm-1 when the zwitterion form is dominant. Another relevant spectral change is
the disappearance of the strong signal at 1037 cm-1 present in the cationic form
spectrum and related to C-N stretching. The CNH deformation, moreover, shifts from
1513 to 1542 cm-1 when the pH is raised. If the comparison is extended to the
spectrum b of L-Met at pH 5.5 (close to isoelectric point), however, identifying
simple tendencies in the alteration of the SER spectrum shape of many bands
becomes problematic; which is reflected in the range of shifts for Met reported by
others [IV.9, IV.10, IV.31]. The concurrence of possible conformers (TG, GT, TT and
GG [IV.31]) for L-Met produces a sequence of closely-spaced vibrational bands
which often overlap according to the shifts caused by the different environment
acidity. A thorough examination of multiple contributes was attempted by Lee et al.
[IV.32] by deconvolution of the broad bands through Fourier Transform analysis.
While such a deconvolution is beyond the scope of this work, it is important to note,
that the proposed method yields spectra with several of the characteristic bands for
this amino acid. The reported spectral fingerprints are, indeed, correspondent to the
ones mentioned by the cited authors for L-Met (Table 2).
Distinguishing two amino acids.
In addition to the simple amino acids solutions, mixtures were investigated. For
examples, L-Met and L-Phe solutions (10-3 M) were mixed in equal volumes before
being deposited with the usual method onto the dried silver colloid. This more
complex sample is produced in order to test a more challenging situation, in which
vibrational bands arising from different components of the mixture fall in
126
neighbouring frequencies. In Figure IV.9, a sufficiently well-defined spectrum of
both amino acids allows the assignment of vibrational bands associated with L-Met
and L-Phe, despite the broadening effect related to SERS: the bands at around 450
cm-1, as well as those at 528, 646, 681, 717, 960, 1091, 1130, 1506 and 1650 cm-1 of
L-Met are clearly distinguishable from those of L-Phe, and only some minor shifts
are observed in the mixture with respect to the SER spectrum of L-Met (Fig IV.7 b).
While the CC ring deformation band at 1004 cm-1 is recognizable in both Fig IV.7a
and Fig IV.9, other bands ascribed to L-Phe occurring at 859 (CC stretching), 1031
(CH stretching), 1207 (phenyl group stretching), 1275, 1357 (COO- stretching),
1418 cm-1 [IV.30, IV.33] are also observed in the L-Met:L-Phe mixture.
127
Fig. IV.8. Three spectra for methionine recorded at different pH values. From top to bottom, pH = 3.5,
pH = 5.3 and pH = 6.8. The upper spectra have been vertically shifted for clarity.
Fig. IV.9 SER spectrum of the mixture L-Met: L-Phe. 10-4 M after drying on the silver nanoparticles
layer. The vibrational bands of Methionine are written in bold, whereas the Phenylalanine spectral
fingerprints are written in italic.
128
Towards a more complex sample.
Fig. IV.10. Molecular structure of Glutathione (γ-L-glutamyl-L-cysteinylglycine)
Glutathione (γ-L-glutamyl-L-cysteinylglycine) provided an example of a naturally
occurring tri-peptide. Analysis of this larger molecule was performed on a droplet of
a 10-4 M solution, dried on the evaporated Ag-LM colloid. In this case the Raman
spectrum of the crystalline powder is provided (fig. 7) to show how the abundance
of bands in the Raman spectrum of the molecule in its solid form is substituted by
fewer, albeit wider, spectral features in the SER spectrum. This phenomenon can be
ascribed to the loss of order occurring when the Glutathione was dissolved in water
[IV.3]. Despite the significantly lower resolution of this SER spectrum, it is possible
to trace many of the vibrational modes of the molecules: 447, 622, 678, 760, 796,
925, 1050, 1281, 1326, 1367, 1634 cm-1, which are assigned in Table IV.4 [IV.28,
IV.34]. Again the most intense spectral features of Glutathione appear at around 650,
1000 and 1300 cm-1. A higher signal to noise ratio is obtained with respect to the
comparable work of Larsson and Lindgren, who used a laser in the NIR range but
gold colloid as the metal substrate [IV.34].
129
Fig. IV.11. SERS (a) and Raman (b) spectra for Glutathione. The spectrum a was recorded with 50x
objective, 5 s acquisitions (10 accumulations) and a laser power of 15 mW; spectrum b was obtained
with 10 accumulations, 20s each, laser power 7.5 mW and 20x obj.
IV.5 Perspectives.
The employed technique (SERS on dried mixtures) and instrument were
remarkably effective in the detection of simple molecules such as amino acids,
independently of the features of their side chains. The proposed method, however, is
intrinsically limited for the identification of more complex molecules or mixtures.
Even if many of the spectral fingerprints can be recovered after the addition of silver
colloids, the overall shape of the spectra is altered. First of all, sequences of closely
spaced narrow bands in the Raman spectrum of the molecules in crystalline form
become a single wide band when diluted. Even if the sample is dried after mixing
with the silver nanoparticles, the “fine structure” of the vibrational spectra is not
fully recovered, resulting in more ambiguous identification of specific spectral
features. This broadening of the Raman bands cannot be assigned to the resolution
of the instrument, which remains the same for the two measurements. It is worth
considering, in further analyses, the effect of the different kinds of synthesized
substrates with the dry approach, to investigate if gold colloids or Ag-HA
130
nanoparticles give a better spectral resolution, even if the enhancement factor, as
previously stated, is on average lower.
More generally, however, the main issue of this technique is the distortion of the
spectral profile which often affects the data obtained , even in the same sample.
These variations in intensity, which do not affect the spectral position of the main
vibrational bands, are caused by the strong dependence of the enhancement on the
local size of the nano-features of the surface [IV.35]. It is well-known that only those
molecular components that are sufficiently close to the SERS active surface (within
∼10 nm) and that have certain spatial orientation can be enhanced [IV.36]. Indeed,
the SER effect can occur if the resonance frequency of the excited SP matches that of
the scattered electric field [IV.37]. A more homogeneous colloid can be obtained by
controlled synthesis involving, for instance, the presence of a salt (NaCl) as an
aggregating agent. The adoption of larger nanoparticles, or of a regularly-shaped
metal matrix may lead to much more predictable behavior of the enhancement
factor, but the choice of the period of the structure must be tailored for a specific
application. The same amino acids in solutions of different pH are currently under
analysis; furthermore, substrates prepared by lithography are being tested in order
to obtain a more uniform substrate and more uniform spectra. Other spectral
distortions could be resolved by using a polarization-resolved device, which would
help to correlate the intensity of a selected Raman band with the direction of the
exciting electric field. Other procedures to address the problem of reproducibility
related to the SERS effect have been proposed, such as averaging of SERS spectra,
using a low magnification objective lens [IV.38] or increasing the colloidal
concentration [IV.31]
Considering the limits and the possible improvements, the current setup showed
that a meaningful analysis of amino acids and peptides present in trace
concentrations can be performed even in absence of advanced laboratory
instruments. The aim of this work was to demonstrate the possibility of adapting a
portable Raman instrument to the SERS analysis of simple organic molecules: this
task was accomplished with careful optimization of the most accessible parameters,
such as the optical components and the fabrication of the metal substrate. The
choice of suitable optics combines the flexibility given by optical fibers to the high
resolution and light collection provided by a microscope objective; the adoption of
131
easy-to-prepare metal colloid must be seen as a preliminary medium to test the
SERS effect on different materials, and it can be replaced by more application-
focused substrates in the future. A more extensive test of both the dry technique and
the portable instrument is planned: if positive results are confirmed, application of
SERS as an in situ diagnostic tool for archaeological and conservation researchers is
foreseen [IV.1]. An important challenge that remains to be investigated is to what
extent one can extract information concerning the nature of archaeological organic
or bio-organic residues through SERS analysis. Searching for specific spectral
signatures that can be correlated with certain materials and/or exclude the presence
of others is a key issue. As indicated above, the use of special preparations of
nanoparticles could potentially lead to SERS analysis based on material specific
enhancement. Additionally the use of chemometrics methods may turn out to be of
importance in screening among different types of residues [IV.39, IV.40]
132
Frequency (cm-1) Frequency SERS (cm-1) Proposed Assignment Bibliographic source
455 480 In phase (C–C–C) [IV.29]
523 521 τ NH3+ , τ NH2) [IV.29]
614 602 In phase (O–CO) [IV.29]
670 662 ω COO ) [IV.29]
721 721 ρ CH2) [IV.29]
796 808 ρ NH2) [IV.29]
898 918 skeletal ν CC , ν CN) [IV.29] [IV.3]
971 964 ρ CH2) [IV.29]
1000 1007 ω CH2) [IV.29]
1050 1050 ω NH3) [IV.29]
1071-1089 1081 ν CN [IV.3]
1138 1130 ρ NH2) [IV.29]
1219 1213 ω CH2) [IV.29]
1315 1314 CH2 ,τ CC [IV.3]
1360 1349 τ CH2) [IV.29]
1442 1444 CH2) [IV.3]
1602 1583 NH2) [IV.29]
1643 NH2) [IV.29]
1703 ν COO ν C=N , NH3+) [IV.29]
Table IV.1. Frequency shift and relative assignment for the detected Raman and SERS bands of L-
Arginine. In this and in the next tables, - deformation, ω - wagging, ρ - rocking, τ - twisting, ν -
stretching.
133
Frequency (cm-1) Frequency SERS (cm-1) Proposed Assignment Bibliographic source
416 410 CCN [IV.9]
450 451 τ NH3) [IV.9]
543 530 CCO [IV.9]
644 644 ν CS CCO [IV.9] [IV.3]
682 660-686 ν CS CCO [IV.9] [IV.3]
719 738 ν CS [IV.9] [IV.3]
767 777 ν CS [IV.9]
804 805 CCH [IV.9]
877 860 ν CC CNH [IV.9] [IV.3]
951 950 ρ CH3) [IV.9]
986 980-987 ν CN [IV.9]
1032 1028 ν CC [IV.9]
1040 ν CN [IV.9]
1071 1068-1078 ρ NH3) [IV.9] [IV.3]
1121 1128 ρ NH3) [IV.9]
1150 1150 CCH [IV.9]
1180 1186 CCH [IV.9]
1250 1243 CCH SCH [IV.9] [IV.3]
1260 1264 -1280 CCH SCH [IV.9] [IV.3]
1322 1318 SCH CH3) [IV.9] [IV.3]
1353 1362 1365 CH2) [IV.9] [IV.3]
1412 CC ν CO [IV.9]
1418 1425 CH3) [IV.9] [IV.3]
1445 1450 ν CC [IV.9] [IV.3]
1510 1506-1513 ν CNH [IV.9]
1628 1623 NH3) [IV.9]
Table IV.2. Frequency shift and relative assignment for the detected Raman and SERS bands of L-
Methionine
Frequency (cm-1) Frequency SERS (cm-1) Proposed Assignment Bibliographic source
622 644 ν Ring [IV.30]
855 858 ν CC – Ring) [IV.30]
913-953 931 C-COO- ) [IV.30,IV.33]
1003 1003 CC – Ring) [IV.30,IV.33]
1036 1031 ν CH , ν Ring [IV.30,IV.33]
1128-1187 1151 CCN asymm [IV.33]
1215 1205 ν Phenyl group [IV.30]
1340 1357 COO-) [IV.30,IV.33]
1411 1418 COO-) symm [IV.33]
Table IV.3. Frequency shift and relative assignment for the detected Raman bands of L-Phenylalanine
134
Frequency (cm-1) Frequency SERS (cm-1) Proposed Assignment Bibliographic source
447 447 ν OH-) [IV.34]
622 622 CS [IV.28]
660 644 CS [IV.28][IV.34]
678 678 CS [IV.28]
737 COO-) [IV.28]
774 765 COO-) [IV.28][IV.34]
811 795 ν COO-) [IV.28]
830 830 C-CN) [IV.28]
920-932 925 C-COO-) [IV.28]
1039 1050 CN [IV.28]
1285 1281 Amide III [IV.28]
1367 1367 COO-) [IV.34]
1445 1448 CH [IV.34]
1632 1634 Amide I [IV.28]
Table IV.4. Assignment for some of the observed Raman bands of Glutathione
135
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CHAPTER V
CONCLUSION.
The common goal of the reported work is to pioneer a new generation of Raman
spectrometers, particularly suitable for the analysis of works of art, thanks to the
mapping approach, but which could also find application in geology or security
controls, for example. The knowledge of the scattering phenomenon on which
Raman spectroscopy is based, together with an in-depth study of the light path
helped us in the determination of the parameters which best fitted the requirement
of a good collection of the signal; most of all, the know-how of a research group
which is well-trained in the application of optical methods of analysis for the study
of Cultural Heritage has guided the construction of an instrument that could match,
as far as possible, the need for a new diagnostic tool. The combination of a near-
infrared laser, which supplied a small but rather powerful light source without the
risk of exciting excessive luminescence, an optical system tailored for the particular
application, the scanning mirrors and the flexibility that the optical fibers give to the
instrument’s layout result in a ductile mapping spectrometer, which covers a niche
in the applications of Raman spectroscopy that was previously unfulfilled.
The Remote Raman Scanner developed as part of this thesis proved to be a suitable
non-invasive diagnostic instrument on a variety of different samples. Tests of
traditional pigments (lead white, ultramarine blue, gypsum and vermilion) on the
model panel, on luminescent white pigments and a modern dye-based yellow
pigment provided good spectra which could be used for material identification,
even though the adoption of a stand-off layout radically decreases the collection
cone of the instrument with respect to a traditional Raman set-up. The result is that
good quality spectra often require acquisition time of the order of a few minutes,
and consequently the background affecting the baseline of the spectrum can be
significant. Nonetheless, the identification of the most intense bands of almost all the
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studied inorganic materials was unambiguous. Moreover, the method for
reconstructing the spectral maps of the target surface, whose application on the
study of minerals has been reported, and is virtually independent of baseline
distortions, thanks to the interactive subtraction of the baseline.
The reconstruction of the intensity profile of the distinguished Raman bands on the
surface under the field of view is the main analytical tool offered by this instrument.
Even if the raster scan of the selected area might be the default choice for probing a
sample, this time-consuming procedure makes the selective analysis a preferable
option: the flexible mapping of the mineral, reported in section III.7 shows how
meaningful information can be extracted by a selection of points, without the need
for a full scan of the area of interest. The multi-analytical approach exploited for the
analysis of the model panel (paragraph III.3) permitted to further limit the number
of needed acquisitions, thanks to the preliminary analysis carried out with
reflectance imaging and X-Ray fluorescence. Of course, the analysis of a surface
depends on the particular application; for this reason, the software control allows a
multiple operation mode (single shot, multiple points with a fixed exposure time,
multiple points with automatic exposure) in order to fulfill specific working
requirements.
The mapping mode has not been applied to the study of the Grillo telephone,
because the spectra collected from different positions on its surface did not show
any significant change. The instrument did not provide any information other than a
confirm for its chemical composition, though, the possibility of performing this
analysis without moving the sample along the field of view plane, and, especially,
along the focal axis, would have been impossible without the peculiarity of Remote
Raman Scanner. The analysis of three-dimensional objects is, thus, possible in a
particularly easy mode.
An application of the system to the analysis of works of art in situ has yet to be
carried out and it is hoped that this will occur in the near futureNonetheless, the
analysed samples and materials have not been treated before the measurement, nor
particular adjustments have been taken when positioning them in front of the
collecting lenses: the long depth of field of the optical system, together with the
robust assembly of the probe give us a solid confidence that the performance on site
would not be so much different from those obtained in laboratory. On the other
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hand, the drawback of the non-contact approach is the need for working in the dark.
The possibility to test two other mobile Raman instruments, currently off-the-shelf,
revealed that the performances of the Remote Raman scanner, on the shown
samples as well as on other standards, are not inferior to the commercially available
counterparts. Of course, some of the ultimate portable Raman spectrometers
provide a better spectral resolution and they are often packed in a more compact
and lighter housing: however, none of these is able to work in a non-contact mode,
nor can they map a surface without a relative movement of the sample. With respect
to the traditional choice of a microscope objective or a short-focal lens as the
terminal optical feature, the long-focal optical system here described, which focuses
the laser beam on a relatively wide spot and therefore deliveries a lower density of
power on the target, presents a reduced risk of damaging the sample.
The work on the surface-enhanced Raman technique employed for helping the
detection of diluted amino acids aims can be seen as a complementary activity in
applying novel techniques for in situ Raman analysis. Not all the issues of this
analytical method can be solved by engineering work on the measurement device,
therefore it is important to carefully evaluate all the other parameters concerning
the measurement as a whole, before to consider it unfeasible. The application of
SERS is a powerful resource to overcome the detection limit of Raman spectroscopy
with organic materials, especially when, as in the cited case of archaeological
vessels, they are present in very low concentrations. This technique is currently one
of the most popular means for the screening and identification of molecules; many
efforts are directed to the development of new materials as substrates which may
grant reproducible spectra. Together with the improvements in the technology for
the detection of optical signals, the possibilities of developing advanced Raman
instruments and methods are in the air. For this reason, it is essential to be ready to
take advantage of the latest discoveries in order to progress in this interesting and
challenging research field.
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Acknowledgements.
I wish to thank prof. Cubeddu for giving me the opportunity of undertaking this PhD;
I thank the former and the current coordinators of the PhD course, respectively prof.
Ciccacci and. prof. Taroni. All my gratitude goes, of course, to my supervisor, prof.
alentini, and to his team: dr. Comelli and dr. Nevin, first of all, but also dr. ’ ndrea,
dr. Osticioli and all the other members of the research group: prof. Pifferi, prof.
Torricelli, dr. Farina, dr. Bassi, dr. Contini, dr. Spinelli, dr. Dalla Mora. I would like to
remember each occasion in which I have been helped by you but I think there is no
space for 140 pages more.
A deserved acknowledgment to my Greek hosts, prof. Fotakis, prof. Anglos and Dr.
Philippidis, for welcoming me in Crete despite the gloomy period.
I feel very grateful towards the researchers and PhD students who collaborated with
this project, and who permitted me to perform the measurements which are here
reported: thanks to Iacopo Osticioli, Austin Nevin, Ilaria Bargigia, Anna Cesaratto,
Francesca Toja, Emanuela Nolfo, Sabrina Moneta, Lucia Ferrario, Iwona Zmuda-
Trzebiatowska and Kristalia Melessanaki.
This is not only the end of the thesis, but also the end of a wonderful period at
Politecnico di Milano. This acknowledgement, therefore, is addressed to everyone
who made me feel at home there. Thank you, I will remember you all.