inelastic neutron scattering and applications · an msa short course on neutron scattering in earth...
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Inelastic Neutron Scatteringand Applications
A Short Course on Neutron Scattering in Earth SciencesDec 7-8, 2006
Hilton Garden Inn, Emeryville, CA
Chun Loong, IPNS
Bay Bridge underconstruction 1936
D.P.Mitchell and P.N.Powers,Phys. Rev. 50 (1936) 486.
2An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
An Outline
The Technique of Inelastic Neutron Scattering (INS)Double differential cross sectionInstruments: Triple-axis vs. TOF chopper spectrometers
Applications of INS in Earth SciencesLattice dynamics: phonon dispersion & density of statesMagnetic scattering: rare-earth energy levels structures
Examples:Xenotime (RPO4)SpinelsNanostructured bone minerals (hydroxyapatite)
Resources: Web, software, text, review
3An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
What is Inelastic Neutron Scattering (INS)? Scattering processes whichinvolve energy and momentum exchange between the neutron & the scatterer
rQx= k0 ! k1 sin" cos#
! k0sin" sin#Qy=
! k1cos#Qz=
E = E0! E
1=
h2
2mnk0
2 ! k1
2( )rQ =
rk0!rk1
The goal is to measure precisely thedouble differential cross section:
!
d2"
d#dE=
1
N
$
% &
'
( )
k1
k0
mn
2*h2
$
% &
'
( )
2 r k
1+
1V
r k
0+
0
2
, E + E+ 0- E+ 1
( )
=k
1
k0
Sr Q ,E( ),
The scattering function,depending on coherent or incoherentscattering, is related to respectively theinter-particle or self-particle space-timecorrelation functions of the scattererunder study.
!
Sr Q ,E( ),
4An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
What Does an INS Instrument Do?Performs Accurate Measurements of S(Q,E) in Absolute Units
In order to differentiate the netenergy change for a scatteringevent, an energy filter, whichselects neutrons with a narrowdistribution of energies and/orspins over a collimated solidangle, has to be inserted in theincident or scattered beam,sometimes in both places.
• For fixed incident energy +variable scattered energies:direct geometry
• For variable incident energy+ fixed scattered energy:inverse geometry
Crystal monochromators
or analyzersand
Choppers
5An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
How to Define the Energy of a Neutron Beam? Crystals & Choppers
6An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
How INS Instruments Work? Triple-Axis Spectrometers
LLB-T2
http://www.nobel.se/physics/laureates/1994/index.htmlhttp://www.science.ca/scientists/scientistprofile.php?pID=4 (3 of 4
Bertrand N.Brockhouse’soriginal TAS(1959)
7An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
!
r k 1
!
"r k 1
!
r Q =
r k 0"
r k 1
!
r k 0
!
"r k f
!
r k
i
!
r k 1
!
r k 0
!
r G
!
r q
!
"r k 1
!
r Q =
r G +
r q ; q " reduced wavevector
!
r Q =
r k 0"
r k 1
!
r Q =
r k 0"
r k 1
E = h# =h2
2mn
r k 0
2
"r k 1
2( ) = E0" E
1
Scattering TriangleConservation of momentum & energy
Operation Modes:Fixed E0 or E1
May keep Q or E constant
How Does a Triple-Axis Spectrometers Work?
8An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
!
" 2# coh
"$"E1
%k
1
k0
F(r Q ,
r q , j)
r q , j
&2
n j (r q ) + 1
2± 1
2[ ]' E0( E
1m E(
r q )[ ]'
r k
0(
r k
1(
r G (
r q [ ],
F(r Q ,
r q , j) ) Inelastic structure factor for one ( phonon coherent scattering
=h
2
2m* E j (r q )
+
, -
.
/ 0
*
&1
2
bcoh
*e(W* (
r Q )
e(i
r Q •
r x (* )
r Q •
r e *;
r q , j( )[ ]
-k1k0
E
qq0Intensity
Resolutionfunction
G. Shirane, S. M. Shapiro, & J. M. Tranquada, Neutron Scattering with a Triple-Axis Spectrometer: Basic Techniques (Cambridge, 2002).
How to Measure Phonons Using a Triple-Axis Spectrometer?
9An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
E. Fermi, W. J. Strum, & R. G. Sachs, “A thermal neutron velocity selector and its application to the measurement of thecross section of boron”, Phys. Rev. 72, 193 (1947).http://www.anl.gov/OPA/logos20-1/fermi01.htm
!
"s = 6d
2r#$ x (%),
$ x
2(%) =
1
10
5 &128% 4
3& 8% 2
'
( )
*
+ , , for 0 - % - 1
4
8
5% &%( )
2 4 + %
2 + %
'
( )
*
+ , , for 1
4- % -
undefined, for % .1
/
0
1 1 1
2
1 1 1
1
% 3r
2#
d
1
vopt&
1
v
'
( ) )
*
+ , , , vopt = 24#.
ω
r
d
Transmission of a single slit -A triangle of Γs in time
Transmission of a slit package - A trapezoid of an overall with Γ
How INS Instruments Work? Chopper Spectrometers
10An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Incident neutron velocity vi defined by chopperphasing relative to t0 (source emission time)
!
time at sample " ts =l1+ l
2
vi,
A scattered neutron reaching a detector at(l3, φ, θ) at arrival time t has a final speed vf
!
v f =l3
t " ts
, then
E = E0" E
1=
mn
2vi
2 " v f
2( ), and r Q =
mn
h
r v i "
v v f( )
Qx =mn
hvi " v f sin# cos$( ),
Qy = "mn
hv f sin# sin$,
Qz = "mn
hv f cos$.
C.-K. Loong, S. Ikeda, and J. M. Carpenter, "The resolution function of a pulsed-source neutron chopperspectrometer", Nucl. Instrum. Methods A 260 381-402 (1987).
How Does a Chopper Spectrometers Work?
φθ
l3l1+l2
11An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
!
r " k 1
!
r " Q
!
r " " k 1
!
r " " Q
!
r k 0
!
r Q
!
r k 1
!
"
is fixed by the chopper (directgeometry), varies as shown for adetector at a scattering angle . Ingeneral, does not follow asymmetry direction in the reciprocalspace for a crystal setting.
!
r k 1
!
r k 0
!
"
!
r Q
M. Arai, “Dynamic structure factor of non-crystallineand crystalline systems as revealed by MARI, aneutron chopper spectrometer”, Adv. Colloid InterfaceSci., 71-72, 209 (1997).
How to Measure Phonons/Magnons Using a Chopper Spectrometer?
If a chopperspectrometer is equippedwith large detector bankscovering a wide range ofscattering angles, eachdetector locus will cut adispersion surface atcertain , Thephonon dispersion canbe reconstructed byresembling the properdata points fromdifferent detectors.
!
r Q ,E
12An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Applications of INS: 1. Lattice Dynamics of MineralsPhonon Dispersion Relations
£As q → 0,acoustic branch:
optic branch:
⇒ non-propagating, localizedmode
!
vp = vg = 2Km1
+m2
a = vsound
!
vg = 0
£Born-von Kámán model with identical force constants from nearest-neighbor interaction
Phase velocity
!
vp ="q
Group velocity*
!
vg = d"dq
Acoustic Mode
Optic Mode
Mass ratio = 2.5
Phonon gap
!
h"0
π/2
http://fermi.la.asu.edu/ccli/applets/phonon/phonon.html
qa
*The direction of group velocity is not parallel to the phonon wave vector in an isotropic medium.
13An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Phonon Density of States (DOS), g(ω)
!
g(")d" = number of vibrational frequencies between " and " + d"
For r atomic constituents in N unit cells, total degrees of freedom is 3rN,
!
g(")d"# = fi(")d"i
r
$# = 3rN fi(ω) is the partial phonon DOS of atomic constituent i
Cutoff frequencyPhonon
gap
14An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Phonon DOS & Thermodynamic Properties
!
F =U + 1
2h" + kBT ln 1# e
#h"kBT( )[ ]$ g(")d"
S = kB (n +1)ln(n +1) # n ln(n)[ ]$ g(")d", n = eh"
kBT #1( )#1
CV = kBh"
kBT
%
& '
(
) *
2
eh"
kBT
eh"
kBT #1( )2g(")d"$
!
"V(T) =
#V
V#T=1
BV0
$iCVi(T) %
i
&1
BV0
$CV(T)
!
P = "#F
#V= "
#U
#V+1
V0$ i n + 1
2( )h%g(%&' )d% = Ps " Pphonon,
$ i =# ln% i
# lnV=
Mie-Gruneisen equation of state
Gruneisen parameter for the ith phonon mode
Melting occurs at Tm above whichPphonon > Ps
O. L. Anderson, Equations of State of Solids for Geophysics and Ceramic Science (Oxford University Press, New York, 1995).
A. Navrotsky, Physics and Chemistry of Earth Materials (Cambridge University Press, Cambridge, 1994).
15An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Phonons & Mechanical Properties: The Continuum Limit
For the optic mode, if atoms carry a charge Q, the polarization induced by an electricfield E is
and the dielectric function is
⇒ resonance at in the infrared region.!
P =Q2
2K "m# 2+ $
%
& '
(
) * E
!
" =1+ # +Q2
2K $m% 2
!
"0
= 2Km
Returning to the example of a diatomic chain:At long-wavelength (q→0) limit, lattice to continuum implieselastic wave equationfor the acoustic mode:
!
"# 2u
#t 2=Y
# 2u
#x 2, where
" =m
1+ m
2
2a3
, and Y =K
a=Young's modulus
Likewise for elastic, electro-elastic, and electro-mechanical properties. A. Askar, Lattice Dynamical Foundations of Continuum Theories (World Scientific, Singapore, 1986).
16An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Important References
Bibliography & Compilation of Phonon Spectra• Scattering of Thermal Neutrons, A Bibliography (1932-1974), Complied by A. Larose and J. Vanderwal
(Plenum, New York 1974).
• H. Bilz and W. Kress, Phonon Dispersion Relations in Insulators (Springer-Verlag, Berlin, 1979).
Texts and Review Articles
• Spectroscopic Methods in Mineralogy and Geology, Ed. F. C. Hawthorne, Reviews in Mineralogy, Vol. 18(Mineral. Soc. America 1988).
• P. Brüesch, Phonons: Theory and Experiments I-III (Springer-Verlag, Berlin, 1982, 1986, and 1987).• Dynamical Properties of Solids, Ed., G. K. Horton and A. A. Maradudin, V. 1-7 (North-Holland 1974-1980)• S. Chaplot et al.,”Inelastic neutron scattering and lattice dynamics of minerals”, Eur. J. Mineral. 14, 291
(2002), and R. Mittal et al., “Modeling of anomalous thermodynamic properties using lattice dynamics andinelastic neutron scattering”, Prog. Mat. Sci. 51, 211 (2006).
• E. Burkel, “Phonon spectroscopy by inelastic x-ray scattering”, Rep. Prog. Phys. 63, 171-232 (2000).
17An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
1. Prepare your samples: single crystals (the larger the better) for phonon dispersionand/or polycrystalline sample (the purer the better) for DOS measurements
2. Go to a reliable, high-flux neutron source, see for example �http://www.neutron.anl.gov/
3. Gain access to a world-class neutron spectrometer: Triple-axis and/or chopperinstrument
4. Check the neutron coherent scattering cross sections of the constituent elements,Beware of incoherent scattering and absorption/resonance. See, for example, http://www.ncnr.nist.gov/resources/n-lengths/
5. Better (necessary for single-crystal experiments) do a group theoretical analysis ofthe neutron spectrum for the crystal structure under study and develop an initiallattice dynamics model to calculate the inelastic structure factor. Software available,for example, L. Warren and T. G. Worlton, "Improved version of group-theoretical analysis oflattice dynamics", Comp.Phys. Commu. 8 71-84 (1974) and J. L. Warren and T. G. Worlton, "Group-theoretical analysis of lattice vibrations", ibid, 3 88-117 (1972). Unisoft: http://134.76.68.210/Eckold/eckold.html, ���Collaborative Computational Project 5: http://www.ccp5.ac.uk/
Incorporate as much as possible data from Raman, IR, Brillouin-scattering,ultrasonic measurements, etc.
Prerequisite for Phonon Experiments Using INS
1. Prepare your samples: single crystals (the larger the better) for phonon dispersionand/or polycrystalline sample (the purer the better) for DOS measurements
18An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Monazite and Xenotime: Rare-Earth Orthophosphates RPO4
Key Collaborators:
J. C. Nipko, Colorado State Univ.L. A. Boatner, Oak Ridge National Lab.M. Loewenhaupt, Tech. Univ. Dresden, GermanyM. Braden, W. Reichardt, Forschungszentrum Karlsruhe, Germany
J. C. Nipko et al., Phys. Rev. B 56 (18), 11584-11592 (1997), & C.-K. Loong et al, Phys. Rev. B 60 (18), R12549-R12552 (1999).
ChemistryHigh melting points (>2000°C)Not attacked by water, organic solvents and common acidsResistant to radiation damage• High-temperature components, Medium for nuclear waste storage
OpticsHigh density, Mohr hardness ~5.5Rare-earth activated luminescence• Phosphors, Lasers, Scintillators
MagnetismAntiferromagnetic phase transitionsCooperative Jahn-Teller effectsMagnetoelastic effectsRare-earth spin-lattice coupling• Magnetic refrigerants, Sensors
Example1
19An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Zircon-type Structure of Nonmagnetic LuPO4 Xenotime
Body-centered tetragonal structure I41/amd Z=2
The Brillouin Zone
36 phonon branches along each direction
Example1
20An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
LuPO4 Lattice Dynamics: Group Theoretical AnalysisExample
1
21An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Single-Crystal, Triple-Axis Measurements of Phonon Dispersion Curves
LuPO4 Room Temperature
Example1
22An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Polycrystalline, Chopper Spectrometer TOF Measurements of Phonon DOSExample
1
23An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
S(Q,E ) =(! r0 )
2
4gJ21" e
"EkT( )
"1
# ' ' (Q,E,T )
$ f2(Q) e
iq•(Ri "Rj)
dt e"iEt /h Ji
%(0)J j
%( t)"&
+&
'i,j
(
S(Q,E) = f2(Q)e
!2W (Q) exp(!Ek /kT )
Zn J" m
2# (En ! Em ! E)
n,m
$
Magnetic INS: The Ground-State Wavefunction of a Magnetic Ion
Magnetic Scattering
Dipole Approximation of Crystal-Field Transitions of Non-interactingRare-Earth Ions in a Crystalline Host
C
B
A
A
B
C
E0
Excitation & de-excitation Observed magnetic-scattering
A
Example1
24An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Crystal-Field Excitation Spectra of TbPO4
A
B
C
TbPO4
E0 = 4 meV
T = 4 K
D
-2 -1 0 1 2 3 4
15 K
60 K
TbPO4
E0 = 20 meV
E, F ,G , I
J, K
D
-1 0 -5 0 5 10 15
15 K
60 K
E, F ,G , I
L,M ,N,O
15 K
50 K
150 K
TbPO4
E0 = 60 meV
J, KP
-1 0 0 10 20 30 40
15 K
50 K
150 K
E (meV)
0 width
8 cm-1 width
Tb sub-lattice
TN=2.2K
TD=2.3K
Example1
D
25An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Crystal-Field Level Structure of TbPO4: The Magnetic Properties
0.0
1.0
2.0
3.0
0 50 100 150 200 250 300
TbPO4
!
(em
u/m
ole
)
T (K)
!//
!"
1.5
2.5
3.5
4.5
0 40 80 120 160 200
TbPO4
2
3
4
4 5 6 7
Specific
heat
(J/m
ole
K)
8 9 10T (K)
TbPO4
calc. CCF
Hill et al.
Specific
heat
(J/m
ole
K)
TN's = 2.28 and 2.15 K
T (K)
The magnetic INS measurement enables a characterization of the rare-earthground- and excited states wavefunctions in terms of a handful of crystal-fieldparameters. The model can then be applied for calculations of the magneticproperties of the material, e.g., susceptibility and magnetic specific heat.
Example1
26An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Anomalous 4f-Electron Phonon Interaction in YbPO4
The coupling of the Yb3+ crystal-field states withthe Eg phonon is very strong, with strengths muchlarger than those of any previously reportedsystems such as CeAl2, LnF3, LiTbF4 and Ln(OH)3.The line widths change drastically withtemperature.
Yb3+ crystal field state
Yb3+ crystal field state
Example1
27An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Dynamic Coupling of Crystal-Field and Phonon States in YbPO4
The data suggest a large fluctuatingcomponent associated with themonopole term whereby coupling ofthe crystal field states, particularlythe upper Γ6 and Γ7 doublets, withphonons of comparable strengthsand energies. The coupling to themonopole term does not require thecompatible symmetry of specificphonon modes (such as in the casefor CeAl2), and was observedthroughout the Brillouin zone aslong as the phonon energies and CFtransition strengths are comparable.
Γ6 Γ7
Example1
28An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Spinels: From Gahnite (ZnAl2O4) to Nanostructured Li(H)Mn2O4 Adsorbent
Koyanaka, Takeuchi, Loong, Separ. Purif. Tech. 43, 9 (2005).Loong & Koyanaka, J. Neutron Res. 13, 15 (2005).
Example2
The classicspinel structure:(e.g., MgAl2O4)Cubic Fd3m,Z=2; 42 phononbranches
Approach:
Synthesis of novel n-MnO2 adsorbents, electronmicroscopy (SEM, TEM), x-ray spectroscopy(EDX & XPS), chemical analysis (ICP) - H.Koyanaka, CRMD/CNRS, Orleans University, France
First-principle molecular-dynamics simulations -C. Fang, University of Uppsala, Sweden
INS - C.-K. Loong, Argonne, USA
29An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Where are the Hydrogen Atoms in HMn2O4?
Ab initiocalculation of H-vibrational frequencies
A proton prefers thetetrahedral 8a cavitysite but moves to oneof the neighboringoxygen, breaking thelocal symmetry………. Fang & de Wijs (05)
Example2
30An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Bone Minerals: Nanotechnology in Our BodyExample
3
Apatite?
31An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Evidence for the Lack of OH- Ions in Bone Crystals asCompared to Hydroxyapatite (HAp) Ca10(PO4)6(OH)2
Loong, Rey, Kuhn, Combes, Wu, Chen, and Glimcher, Bone 26, 599 (2000).Loong, Thiyagarajan, Kolesnikov, Nanotech. 15 S664 (2004).
Approach:
Preparation of deproteinized bone apatiteCrystals - M. J. Glimcher et al., Harvard MedicalSchool, USA
Synthesis of hydroxyapatite powders,Fourier-transform infrared spectroscopy,chemical analysis - C. Rey, CIAIMAT-ENSCT,Toulouse, France
Proton solid-state NMR - Y. Wu, HarvardMedical School, USA
Neutron inelastic scattering & SANS - C.-K.Loong, Argonne, USA
Example3
32An MSA Short Course on Neutron Scattering in Earth Sciences, Dec 7-8, 2006, Emeryville, CA
Concluding Remarks INS is capable of accounting for the detailed atomic/molecular motions and
electronic/magnetic excitations -- individual or collective -- within a many-bodysystem (e.g., minerals).
Since microscopic motions or excitations may occur in vastly different time andlength scales, typically ps to ms and sub-nm to µm, the technique of INSnecessitates an as wide as possible coverage in the energy (E) and wavevector(Q) space with good resolutions. In situ measurements under extreme sampleenvironments (e.g., high T, high P) are highly desirable.
INS is often flux-limited because of the weak intensity but this situation will beimproved in the advent of new-generation high-flux neutron sources such asSNS.
Interpretation of INS data can be a challenge facing experimentalists.Researchers nowadays have to apply methods of theoretical modeling andsimulations that require high degree of sophistication and substantial amount ofcomputing resources.
Don’t worry, instrument scientists at neutron facilities will be glad to help you.