lecture 1: introduction metals, insulators and ...€¦ · metals, insulators and semiconductors...
TRANSCRIPT
1
Lecture 1: IntroductionLecture 1: Introduction
Metals: conduct electricity down to lowest T's
Non-metals: may conduct at ↑T, but cond. ↓ as T↓
Metals, insulators and semiconductorsMetals, insulators and semiconductors
Metallic and nonMetallic and non--metallic solidsmetallic solids
….. can be understood from filling of bands:
E
N(E)band gap
conduction bandvalence
band
E
N(E)Fermi level
EF
Lecture 1: IntroductionLecture 1: Introduction
Conduction in systems with a band gapConduction in systems with a band gap
Metallic and nonMetallic and non--metallic solidsmetallic solids
high T: ionic conductivity (e.g. NaCl)- low cond. cf. metallic conductivity
electronic cond. needs e- excited to the conduction band - thermal excitation (small gap)- optical excitation
= photoconductivity (Xerox)
Lecture 1: IntroductionLecture 1: Introduction
Band picture works fairly wellBand picture works fairly well
Metallic and nonMetallic and non--metallic solidsmetallic solids
ionic system- cation levels empty (e.g. Na+)
- anion levels full (e.g. Cl-)
molecular solid- gap between HOMO and LUMO
Egap
Interesting cases: partially filled orbitals
e.g. transition metal oxides such as ReO3 has (5d)1
metallicsometimes TM-O NOT metallic (interesting…!)
Lecture 1: IntroductionLecture 1: Introduction
Many properties depend on thermal excitation of e- from ground state
No. particles in excited state at temperature T:
ni ∝ exp (- Ei / kT ) Boltzmann distribution
BUT
…….can't use Boltzmann for electrons in a solid !
Metals, insulators and semiconductorsMetals, insulators and semiconductors
Thermal excitation of electronsThermal excitation of electrons
Lecture 1: IntroductionLecture 1: Introduction
Electrons obey the Pauli exclusion principle
Electrons are indistinguishable (exchange of electrons between two occupied levels does not lead to a different arrangement)
Thermal excitation of electronsThermal excitation of electrons
1 + exp [ (E - EF) / kT ]f (E) =
1 FermiFermi--DiracDiracdistributiondistribution
Lecture 1: IntroductionLecture 1: Introduction
T=0: Fermi-Dirac distribution
Thermal excitation of electronsThermal excitation of electrons
1 + exp [ (E - EF) / kT ]f (E) =
1 FermiFermi--DiracDirac distributiondistribution
f(E
)
E
top filled level in band = EF
filled empty
these states determine a number of properties: e.g. electronic specific heat
Fermi-Dirac distribution can be measured directly using photoemission
f(E
)
Energy
T=0 < T1 < T2
increase T:
2
Lecture 1: IntroductionLecture 1: Introduction
Thermal excitation of electronsThermal excitation of electronsFermiFermi--DiracDirac distributiondistribution
f(E
)
Energy
Width ca. 4 kT
4kT
room temp. 4kT is ca. 0.1 eV
Total width of bands often eV
only small no. of total e- are thermally excited
Fermi level is fundamental: it's the thermodynamic chemical potential for e- in the solid
Metals in contact: charge transferred till EF's are equal
Lecture 1: IntroductionLecture 1: Introduction
SemiconductorsSemiconductors
Non metals
conduct via thermal excitation of carriers across gap
Metals, insulators and semiconductorsMetals, insulators and semiconductors
missing e- in valence band (holes)
e- in the conduction band
Egap ca. 1 eV
Lecture 1: IntroductionLecture 1: Introduction
SemiconductorsSemiconductors
Fermi level now lies in the gapThermal excitation of electronsThermal excitation of electrons
VBCB
pure solid
n-type
p-type
Fermi-Diracdistribution
EF
EF
EF
Lecture 1: IntroductionLecture 1: Introduction
SemiconductorsSemiconductors
Bottom of conduction band:
E - E F = E gap / 2
E - E F usually much larger than kT
exponent dominates
no. of exited electrons: n ∝ exp (-E gap / 2kT)
Thermal excitation of electronsThermal excitation of electrons
1 + exp [ (E - EF) / kT ]f (E) =
1
cf. intrinsic behaviour of pure materialsArhheniusbehaviour
A course given as part of the joint Masters programmeA course given as part of the joint Masters programme
Condensed Matter ScienceCondensed Matter Science
of the Universiteit van Amsterdamof the Universiteit van Amsterdamand the and the VrijeVrije Universiteit, Amsterdam.Universiteit, Amsterdam.
Mark Golden (Mark Golden (UvAUvA) & Bernard Dam (VU)) & Bernard Dam (VU)
Electronic Structure and Chemistry of SolidsElectronic Structure and Chemistry of Solids
Lecture 2: Spectroscopic Methods
Mark S. Golden, Van der Waals-Zeeman Institute, Universiteit van Amsterdam, Room 2.09, Valckenierstraat 65, 1018 XE Amsterdam, Tel.: 020 525 6363.
[email protected] http://www.science.uva.nl/research/wzi/cmp
Electronic Structure & Chemistry of Solids (2005)Electronic Structure & Chemistry of Solids (2005)
Book chapterBook chapter lecturer date(s)lecturer date(s)
• Introduction - MSG 30.10• Spectroscopic methods - MSG 03.11• Electronic energy levels and chem. bonding - BD 07.11, 10.11• Optics (not in Cox as such [i.e. better]) - BD 14.11• Elementary band theory - MSG 17.11, 21.11• The effects of electron repulsion - MSG 24.11, 28.12• Lattice distortions - BD 08.12• Defects, impurities and surfaces - BD 15.12• Questions and answers session - all 19.12
• Closing workshop with presentations - all 22.12.2005• Oral exams - all Jan. 2006
3
Question from Lecture 1: Intro, bonding, classification of solidQuestion from Lecture 1: Intro, bonding, classification of solidss
Discuss the different types of bonding encountered in the alkaliDiscuss the different types of bonding encountered in the alkali metal metal intercalated Cintercalated C6060 compound Kcompound K33CC6060..
This is a soThis is a so--called called fulleridefulleride, has an , has an f.c.cf.c.c structure and is a metal and a structure and is a metal and a superconductor (superconductor (TcTc 18K). There is charge transfer from the K atoms to the C18K). There is charge transfer from the K atoms to the C6060cages.cages.
© s
teph
en.h
eyes
@ch
em.o
x.ac
.uk
© J.W. Bullard, 1999
http://rs1.physik.uni-dortmund.de/sem/c60/kap6.htm
Lecture 2: checkLecture 2: check--up of Lecture 1 materialup of Lecture 1 material
Importance of solidsImportance of solids
Molecular solidsMolecular solidsIonic solidsIonic solidsCovalent solids Covalent solids Metallic solidsMetallic solids'Real', complex solids'Real', complex solids
Chemical classification of solidsChemical classification of solids
OrbitalsOrbitals in atoms, molecules and solidsin atoms, molecules and solidsBands and bondsBands and bonds
Electrons in solidsElectrons in solids
Metallic and nonMetallic and non--metallic solidsmetallic solidsThermal excitation of electronsThermal excitation of electronsSemiconductorsSemiconductors
Metals, insulators and semiconductorsMetals, insulators and semiconductors
OK ?
Lecture 2: Spectroscopic methodsLecture 2: Spectroscopic methods
IntoductionIntoduction: types of (electronic) spectroscopy: types of (electronic) spectroscopy
General principlesGeneral principlesApplications of PESApplications of PESInverse PESInverse PES
PhotoemissionPhotoemission
General principlesGeneral principlesApplications of xApplications of x--ray emission spectroscopyray emission spectroscopyXX--ray absorption spectroscopyray absorption spectroscopy
XX--ray spectroscopyray spectroscopy
Band gaps and Band gaps and excitonsexcitonsAbsorption and reflectivityAbsorption and reflectivityMetals Metals -- the plasma frequencythe plasma frequency
Optical propertiesOptical properties STM / STSSTM / STSGeneral principlesGeneral principlesApplications of STMApplications of STM
not in Cox
Bernard: later
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Spectroscopic methodsSpectroscopic methods
to understand the electronic properties, we need to to understand the electronic properties, we need to learn about the electrons in a solidlearn about the electrons in a solid
spectroscopy can tell us about what the electrons are spectroscopy can tell us about what the electrons are doing in real materials doing in real materials
energy
momentum
spin1023 electrons
EM-radiation electrons
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
A warmA warm--up 'competition':up 'competition':
take 2 minutes to write down as many spectroscopic take 2 minutes to write down as many spectroscopic methods as you can think of that involve the electronic methods as you can think of that involve the electronic and optical properties of a solidand optical properties of a solid
(using, for example electrons/radiation as incoming and (using, for example electrons/radiation as incoming and outgoing 'particles')outgoing 'particles')
1023 electrons
EM-radiation electrons
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Types of spectroscopyTypes of spectroscopy
Probing particles:Probing particles: Method:Method: Information about:Information about:
Photon in, electron outPhoton in, electron out PES PES occupied statesoccupied states
Electron in , photon outElectron in , photon out IPESIPES unoccupied statesunoccupied states
Photon in, photon outPhoton in, photon outxx--raysrays XES, XES, RIXSRIXS occupied statesoccupied statesvisible light, IRvisible light, IR reflectivity,reflectivity, conduction electronconduction electron
ellipsometryellipsometry dynamicsdynamics
Photon inPhoton inxx--raysrays XASXAS unoccupied statesunoccupied statesvisible light, IRvisible light, IR absorptionabsorption band gap, defect statesband gap, defect states
Electron in, electron outElectron in, electron out EELSEELS collective excitationscollective excitations
Electron in Electron in oror electron outelectron out STM / STSSTM / STS occupied or unoccupied occupied or unoccupied states (local)states (local)
4
PES XPS IPES XAS AES EEPES XPS IPES XAS AES EELSLS
NN--11 NN--11 N+1N+1 N, N, can becan be≈≈ N+1N+1
N N NN--22
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
photoemissionphotoemissionoror
photoelectron spectroscopyphotoelectron spectroscopy
conceptually very simpleconceptually very simple
Pedestrian guide to PESPedestrian guide to PES
KE = hν - BE binding energy of the electron in the crystal
kinetic energy of photoelectron in the vacuum
theoretical beginnings:theoretical beginnings:
Albert Einstein at beginning of 20th century (Albert Einstein at beginning of 20th century (→→ Nobel prize)Nobel prize)
experimental beginnings:experimental beginnings:
Heinrich Hertz at end of 19th centuryHeinrich Hertz at end of 19th century
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
step 1step 1
incoming photon causes an incoming photon causes an
optical transition in the solidoptical transition in the solid
'vertical' transition'vertical' transition
simplesimple
Three step model for PESThree step model for PES
purely phenomenological, but usefulpurely phenomenological, but useful
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
simplesimple
Three step model for PESThree step model for PES
step 2step 2
transmission of the photoelectron through the solid transmission of the photoelectron through the solid
(towards surface)(towards surface)
energyenergy--loss processesloss processes
secondary electronssecondary electrons
inelastic mean free path, inelastic mean free path, λλ
purely phenomenological, but usefulpurely phenomenological, but useful
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
simplesimple
Three step model for PESThree step model for PES
step 3step 3
transmission of the photoelectron across the surface transmission of the photoelectron across the surface
and into the vacuumand into the vacuum
through surface potential barrierthrough surface potential barrier
kk⊥⊥ not conservednot conserved
purely phenomenological, but usefulpurely phenomenological, but useful
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
5
Ener
gy
Ener
gy →→
(1)(1) (2)(2) (3)(3)3 step model3 step model
samplesample vacuumvacuum
ΦΦ
EEvv
EEFF
hhνν
photoexcitationphotoexcitation transport to transport to surfacesurface
transmission transmission across surfaceacross surface
secondary secondary electron electron cutcut--offoff
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Kinetic energy Kinetic energy →→
Generic spectrumGeneric spectrum
←← Binding energyBinding energyhhνν--ΦΦsamplesample
hhνν--ΦΦspectrometerspectrometer00
00
hhνν--ΦΦsamplesample
e.g. VB e.g. VB of goldof goldEEFF
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
ΦΦsamplesample
'Fermi edge''Fermi edge'direct measure of direct measure of FermiFermi--DiracDiracdistribution:distribution:
PES is ionising spectroscopyPES is ionising spectroscopy
⇒⇒ in metals:in metals:
if if TTsamplesample low enough, the 10%low enough, the 10%--90% width of the Fermi edge 90% width of the Fermi edge ((≈≈FWHM Gaussian) measures the experimental energy resolutionFWHM Gaussian) measures the experimental energy resolution
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
'Fermi edge''Fermi edge'direct measure of direct measure of FermiFermi--DiracDiracdistribution:distribution:
PES is ionising spectroscopyPES is ionising spectroscopy
⇒⇒ in metals:in metals:
if if TTsamplesample low enough, the 10%low enough, the 10%--90% width of the Fermi edge 90% width of the Fermi edge ((≈≈FWHM Gaussian) measures the experimental energy resolutionFWHM Gaussian) measures the experimental energy resolution
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Surface sensitivitySurface sensitivity cross section for inelastic scattering cross section for inelastic scattering of of photoelectonsphotoelectons during steps 2,3 is during steps 2,3 is HIGH !HIGH !
3λ = 3 nma few atomiclayers !
crystal
photons
KEe,vacuum = hν - BEe,crystal
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
IMFPIMFP
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
inelastic mean free inelastic mean free pathlengthpathlength, , λλ
λλ defined as path length after which transmitted signal = defined as path length after which transmitted signal = 1/e of original signal1/e of original signal
λλ::
•• KE dependentKE dependent
•• weakly material weakly material dependentdependent
'universal' curve'universal' curve
6
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
1) you need photons.....1) you need photons.....
light sourceslight sources
VUV photonsVUV photonsxx--ray photonsray photons
in the labin the lab
synchrotron radiationsynchrotron radiation
21 1486 21 1486 eVeV
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
3rd generation SR sources3rd generation SR sources
BESSY GmbH,BESSY GmbH,BerlinBerlinU125U125--1/PGM 1/PGM beamlinebeamline
Swiss Light Source,Swiss Light Source,PSI, PSI, VilligenVilligen, CH., CH.SIS SIS beamlinebeamline
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
3rd generation SR sources3rd generation SR sources
BESSY GmbH,BESSY GmbH,BerlinBerlinU125U125--1/PGM 1/PGM beamlinebeamline
Swiss Light Source,Swiss Light Source,PSI, PSI, VilligenVilligen, CH., CH.SIS SIS beamlinebeamline
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
intense, brilliantintense, brilliantselectable energyselectable energy
= monochromatic= monochromaticselectable selectable polarisationpolarisation
! VUV: too high E for lasers! VUV: too high E for lasers
! no windows possible! no windows possible
! reflecting optics! reflecting optics
synchrotronsynchrotronsourcessources
Synchrotron radiationSynchrotron radiation
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
1) you need to 1) you need to analyseanalyse the KE and the KE and θ,φ θ,φ
distribution of the photoelectrons.....distribution of the photoelectrons.....
7
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PhotoemissionPhotoemission an advanced PES setan advanced PES set--up works like this:up works like this:
ultrahigh vacuum chamber
photon source
750 k750 k∈∈ Pic: Damascelli
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
what doeswhat does
photoemission measure ? photoemission measure ?
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PESPES
ionising spectroscopyionising spectroscopy
no. of electrons vs. their binding energyno. of electrons vs. their binding energy
'direct' measure of occupied density of states: N(E)'direct' measure of occupied density of states: N(E)
[......ionisation cross sections, polarisation selection [......ionisation cross sections, polarisation selection rules....]rules....]
intensities of different bands in a PES spectrum are weighted by the cross-section of the atomic orbital which makes up the band
tabulated
PhotoionisationPhotoionisation cross sectionscross sections
radial part of the radial part of the wavefunctionwavefunction importantimportant
good match of initial and final state good match of initial and final state wavefunctionswavefunctions
optimal overlap:optimal overlap:
low low EEfinalfinal + extended |i> (e.g. C 2s, 2p)+ extended |i> (e.g. C 2s, 2p)
high high EEfinalfinal + + compact |i> (e.g. C1s)compact |i> (e.g. C1s)
→→ use to use to discriminate between different |i>discriminate between different |i>
final state ! final state ! (selected (selected via choice of via choice of hhνν))
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
examples (Cox and other) of examples (Cox and other) of photoemissionphotoemission
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PES PES and XAS/IPESand XAS/IPES of Cof C6060
PES gives energy PES gives energy distribution of the filled distribution of the filled MO's......MO's......
......or the bands formed ......or the bands formed in the solidin the solid
gas phasegas phase
solid statesolid state
C60: molecular solid !
bands only slightly broader and shifted
8
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PESPESgas phase vs. molecular solidgas phase vs. molecular solid
sharp MO's in gas phase molecule sharp MO's in gas phase molecule broadenbroaden due todue toband formation band formation in the solidin the solid
(not much for solid C(not much for solid C6060 ⇔⇔ superconductivity ?)superconductivity ?)
shiftshift to lower BE in solidto lower BE in solid
= = screeningscreening of 'hole' made by removing photoelectron.of 'hole' made by removing photoelectron.→→ in solid there is extra interin solid there is extra inter--site screening:site screening:
Solid = continuum, relative dielectric constant Solid = continuum, relative dielectric constant εεrr (molecular (molecular polarisabilitypolarisability). ). Insert charge Insert charge qq spread over radius spread over radius rr from vacuum into solidfrom vacuum into solid
→→ electrostatic polarisationelectrostatic polarisation. . For For rr ~ atom, ~ atom, ∆∆E of order 1 E of order 1 eVeV..
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PESPESmetal metal -- valence band photoemission (UPS)valence band photoemission (UPS)
(generally) broad bands(generally) broad bandse.g. VB of aluminiume.g. VB of aluminium
inelastically scatteredelectrons
Fermi-Diraccutoff
E F
N(E) ∝ E½
free-electron band is a parabola
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
angle resolved photoemissionangle resolved photoemission
samplesample
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
metal metal -- angle resolved valence band photoemission (ARPES)angle resolved valence band photoemission (ARPES)
single crystalline sample
angle-reolved detection of photoelectrons
What physical quantities are measured in photoemission ?What physical quantities are measured in photoemission ?
Fermifunction
spectralfunction
vectorpotential(photons)
momentum(photoelectrons)
Spectral function:
the probablility of removing an electron of energy E andwavevector k from the interacting N-electron system
BUT the matrix element is always present:
dependence on photon energy, polarisation....
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
How to determine kHow to determine k||||
momentum component parallel to surface, pmomentum component parallel to surface, p||||
samplesample
KE=½mvKE=½mv22, p=, p=mvmv
KE=½pKE=½p22/m/m
p=(2mKE)p=(2mKE)½½
kk vector parallel to surface, kvector parallel to surface, k||||
θθ sin)2(sin ½|| mKEpp ==
θsin)/2( ½2|||| hh mKEpk ==
vertical transitions and kvertical transitions and k||||--conservation across surfaceconservation across surface
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
9
ARPESARPES
what about kwhat about k⊥⊥? ?
EEii
EEFF
EEkinkin
hhννΦΦ
EEVV
VV00
(w.r.t. bottom of band) electrons feel an attractive (w.r.t. bottom of band) electrons feel an attractive potential, Vpotential, V00 = E= EFF + + ΦΦ
inner potentialinner potential
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
ARPES for 2D systemsARPES for 2D systems
if kif k⊥⊥ not particularly important for the energy variation of not particularly important for the energy variation of the electronic states the electronic states
θθ sin)(512.0sin2|| eVEmEk kin
kin ==h
in Åin Å--11 in in eVeV in in degrees degrees
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
0.00.20.4Binding energy (eV) Momentum (Å-1)
0.3 0.4 0.5 0.6 0.7
EEnergy nergy DDistribution istribution CCurves I (k,E) urves I (k,E) MMomentum omentum DDistribution istribution CCurvesurves
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
StateState--ofof--thethe--art ARPES of a art ARPES of a high high TcTc superconductorsuperconductor BorisenkoBorisenko et al., PRBet al., PRB6464, 094513 (2001) , 094513 (2001)
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
ARPES data - equal footing in either in E or k
EDC - I (kx,ky,E) EDM - I (kx,ky,E)
MDM - I (kx,ky,E)
MDC - I (kx,ky,E)
A full picture of IA full picture of IPESPES vs. the 3D vs. the 3D kkxx, , kkyy, E, EBB spacespace
0.5
eV
(π,π)(π,0)
EF
MX
min max
X
X
YM
M
Bin
ding
ene
rgy
(eV
)
Momentum (Å-1 )
ky
kx
2
EF
BorisenkoBorisenko et al., PRBet al., PRB6464, 094513 (2001) , 094513 (2001)
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Constant energy surfaces: E dependenceConstant energy surfaces: E dependence
KordyukKordyuk et al., 2000et al., 2000300K, 300K, hhνν = 21 = 21 eVeV
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
HTSCHTSC
10
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
time for a coffeetime for a coffee
Lifetimes contd.Lifetimes contd.
ττhh are of the order of 10are of the order of 10--1515 secondsseconds
PES is a PES is a FASTFAST probeprobe
ττhh << << ττee
energy widths in PES are energy widths in PES are dominated by hole lifetime:dominated by hole lifetime:
ee
hh
Lecture 2: Spectroscopic methodsLecture 2: Spectroscopic methods
Self energy and the spectral functionSelf energy and the spectral function
Spectral function:Spectral function:
causes E shiftcauses E shift
causes width causes width ((LorentzianLorentzian))
Lecture 2: Spectroscopic methodsLecture 2: Spectroscopic methods
imaginary part of the self energy
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
core level photoemissioncore level photoemission
Core level photoemissionCore level photoemission
xx--ray ray photelectronphotelectron spectroscopyspectroscopy
NN--11
"XPS""XPS"
core levels strongly core levels strongly localisedlocalised, thus , thus BE'sBE'sgive give elemental identificationelemental identification
chemical shiftschemical shifts give information on:give information on:
* chemical environment of emitter* chemical environment of emitter
* oxidation / valence / bonding state* oxidation / valence / bonding state
satellites satellites and/orand/or shake upshake up are the response of are the response of system to core system to core ionisationionisationangular distribution angular distribution (PhD, XPD) is a local, non(PhD, XPD) is a local, non--destructive structural probedestructive structural probe
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PESPESphotoemission using xphotoemission using x--rays (XPS)rays (XPS)ionise either valence bands or core levelsionise either valence bands or core levelse.g. Nae.g. Na0.70.7WOWO33
BE of core level characteristic for element
11
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PESPESXPS as ESCA XPS as ESCA ''EElectron lectron SSpectroscopy for pectroscopy for CChemical hemical AAnalysis'nalysis'
core level BE signals core level BE signals which elementwhich element
exact BE exact BE cancan give info give info about chemical about chemical environmentenvironment
surface sensitive surface sensitive chemical analysischemical analysis
C atoms in four different surroundings
L. K
arls
son,
Upp
sala
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PESPESphotoemission using xphotoemission using x--rays (XPS)rays (XPS)e.g. Nae.g. Na0.70.7WOWO33
zoom inzoom in
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PESPESusing using photoionisationphotoionisation crosscross--sectionssections
ionise either valence bands or core levelsionise either valence bands or core levelse.g. Nae.g. Na0.70.7WOWO33
hν = Al:Kα (1487eV) He I (21.2 eV)
VBVB
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
inverse photoemissioninverse photoemission
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Inverse photoemissionInverse photoemission
sample a solidsample a solid
monochromatic electron beammonochromatic electron beam
fall into empty electronicfall into empty electroniclevels levels in the solidin the solid
measure:measure:intensity of emitted radiation (intensity of emitted radiation (BremstrahlungBremstrahlung) vs. ) vs.
KE of electrons, orKE of electrons, orintensity and energy of emitted radiation for intensity and energy of emitted radiation for
constant incoming electron energyconstant incoming electron energy
......also surface sensitive & lower resolution than PES......also surface sensitive & lower resolution than PES
sample
N+1N+1
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Inverse photoemissionInverse photoemission
combination PES + IPES is powerfulcombination PES + IPES is powerful1) metals1) metals2) systems with gaps2) systems with gaps
N+1N+1NN--11
transporttransport gap
.....cf. excitonsdiscussed later
12
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PES + IPESPES + IPES
N+1N+1NN--11
TM 3d bandTM 3d band
3d band filling ↑
3d band narrows
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
xx--ray absorption / emission ray absorption / emission & co.& co.
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Core level spectroscopiesCore level spectroscopies
Core Core orbitalsorbitals not directly involved in bondingnot directly involved in bonding
→→ sharp, retain their atomic identitysharp, retain their atomic identityZZ, , angular momentum l angular momentum l
sitesite--selectiveselective & & symmetrysymmetry--selectiveselective spectroscopiesspectroscopies
monochromatic photons, tuned to core level transitionsmonochromatic photons, tuned to core level transitions
requires synchrotron radiationrequires synchrotron radiation
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
times have moved on since ESS was written....times have moved on since ESS was written....
synchrotron radiation sources have become synchrotron radiation sources have become commonplacecommonplace
XAS / EXAFS is XAS / EXAFS is widelywidely usedused
XES is enjoying a renaissance (SRXES is enjoying a renaissance (SR--excited)excited)
XAS & XESXAS & XES
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
xx--ray absorptionray absorption resonant IXSresonant IXS xx--ray emissionray emissionXASXAS RIXSRIXS XESXES
NN--11NNNN ≈≈ N+1N+1
unoccupied excitations vs. q occupied
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Core level spectroscopiesCore level spectroscopies
Simple symmetry selection rulesSimple symmetry selection rules
XASXAS
1) 1s 1) 1s →→ 2p, 2p 2p, 2p →→ 3d3d
2) 1s 2) 1s →→ e.g. 2pe.g. 2pxx for for E E of of hhννinin parallel a axisparallel a axis
XESXES
1) 1s core hole 1) 1s core hole →→ filled from electrons from 2p (3p)filled from electrons from 2p (3p)
2) 2) analyseanalyse E E of of hhννoutout →→ e.g. 2pe.g. 2pxx electrons onlyelectrons only
dipole selction rule
Can be bulk sensitive, can cope well with insulators Can be bulk sensitive, can cope well with insulators ….life sciences….life sciences
13
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PolarisationPolarisation--dependent XES: dependent XES: glycineglycine on Cu(110)on Cu(110)A. NilssonA. Nilsson(Uppsala & ALS)(Uppsala & ALS)
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
PolarisationPolarisation--dependent XAS: Srdependent XAS: Sr22CuOCuO33
O1s
O2p/Cu3d
formally Cu 3dformally Cu 3d99 + O 2p+ O 2p66
covalence (Cu3d/O2p covalence (Cu3d/O2p hybridisationhybridisation) leads to unoccupied O2p states: ) leads to unoccupied O2p states: 'intrinsic' hole states'intrinsic' hole states
Expect:Expect:
O(1):O(2) = 2O(1):O(2) = 2
XAS says = 1.8XAS says = 1.8
VVpdpd pushes pushes holes to holes to
peripheryperiphery
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Core level spectroscopiesCore level spectroscopies
EXAFS: EXAFS: in XAS also scan hν far above the core threshold:
EExtended xtended XX--ray ray AAbsorption bsorption FFine ine SStructuretructure
Outgoing photoelectron = free electronOutgoing photoelectron = free electron
backback--scattering from surrounding atoms scattering from surrounding atoms →→ interferenceinterference
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
EXAFSEXAFS
Interference: outgoing and reflected waves Interference: outgoing and reflected waves →→ EXAFS wiggles EXAFS wiggles in the signal from the corein the signal from the core--ionisedionised sitesite
Depends on:Depends on:
wavelength of free electron statewavelength of free electron state KEKEpathlengthpathlength to and from surrounding atomsto and from surrounding atoms
EXAFS sensitive to local structureEXAFS sensitive to local structure::
sitesite--selectiveselective
long range order not necessary !long range order not necessary !
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
EXAFSEXAFS
O:K edge O:K edge (O1s)(O1s)
GeOGeO22 in:in:
glassyglassy
hexagonalhexagonal
tetragonal tetragonal
structuresstructures
Result:Result:local colocal co--ordination ordination like hexagonal like hexagonal
530 eV in absolute E scale
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
final states can be important in final states can be important in core level spectroscopiescore level spectroscopies
14
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Core level spectroscopiesCore level spectroscopies
Watch out for the core hole !Watch out for the core hole !
IntraIntra--atomic interactions between core hole and other atomic interactions between core hole and other levels can mean that all DOSlevels can mean that all DOS--related info is lostrelated info is lost
e.g. atomic e.g. atomic multipletsmultiplets in TMin TM--LL2,32,3 XASXAS
If adequately dealt with theoretically, these effects can If adequately dealt with theoretically, these effects can be used elegantly be used elegantly →→
e.g. e.g. info on info on valencyvalency and and covalencycovalency ininTM and RE systemsTM and RE systems
Tm is Tm is purelypurelydivalentdivalent
4f4f1313
initial stateinitial state
air stableair stablePESPES Tm4dTm4d→→4f excitations4f excitations
Phys. Rev. Phys. Rev. LettLett., ., 7979, 3026 (1997), 3026 (1997)
Tm@CTm@C8282
Using final state Using final state multipletsmultiplets to determine to determine valenciesvalencies
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
scanning probe methodsscanning probe methodsnow……now……
….. finish off spectroscopic ….. finish off spectroscopic methods with STM/STSmethods with STM/STS
Pic: Crommie, Lutz, Eigler, IBM
Scanning probe microscopyScanning probe microscopy
(i) (i) thought up in 1980's thought up in 1980's ('86 Nobel prize ('86 Nobel prize BinnigBinnig & Rohrer, IBM)& Rohrer, IBM)(ii) (ii) simplesimple(iii)(iii) amazingly flexibleamazingly flexible
plus (bonus): plus (bonus): …..produces sexy, …..produces sexy, colourcolour imagesimages
Scanning tunneling microscopy (STM)
Scanning tunneling spectroscopy (STS)
Atomic force microscopy (AFM)
Magnetic force microscopy (MFM)
…your name….microscopy (XYM)
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Basic principleBasic principle
tiptip
sample surfacesample surface
electronic tunneling from electronic tunneling from 'atomically' sharp tip'atomically' sharp tip
local forces tiplocal forces tip⇔⇔surface surface bend a flexible cantileverbend a flexible cantilever
oror
STM / STSSTM / STS AFMAFM laser
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
15
Scanning tunneling microscopy & spectroscopyScanning tunneling microscopy & spectroscopy
overlap of overlap of wavefunctionswavefunctions: : tip tip ↔↔ samplesample
picspics: Uni. Kiel: Uni. Kiel
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Scanning tunneling microscopy & spectroscopyScanning tunneling microscopy & spectroscopy
picpic: Uni. Kiel: Uni. Kiel
Quantum mechanical tunneling current:Quantum mechanical tunneling current:
κκ -- barrier dep. barrier dep. constantconstant
dd -- distancedistance
For a metal, For a metal, κκ is ca. 1 Åis ca. 1 Å--11
move tip away by 1 Å….move tip away by 1 Å….
...current decreases by ca. 10x...current decreases by ca. 10x
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Scanning tunneling microscopy & spectroscopyScanning tunneling microscopy & spectroscopy
picpic: Uni. Kiel: Uni. Kiel
Q: which electronic states are involved ?Q: which electronic states are involved ?
Q: which direction do the electrons tunnel ?Q: which direction do the electrons tunnel ?
A: those of A: those of bothboth tip and sample surfacetip and sample surface
--++
++
--
A: depends on the biasA: depends on the bias
unoccupied occupied statesunoccupied occupied states
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Scanning tunneling microscopy & spectroscopyScanning tunneling microscopy & spectroscopy
Feedback loop: keep Feedback loop: keep II tt
constant while moving constant while moving tip in x and ytip in x and y
topologytopology
Feedback off: constant Feedback off: constant height and measure height and measure II tt
vs. vs. VV biasbias
spectroscopyspectroscopy
STMSTM
STSSTS
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
STM as tool for atomic sculpture…..STM as tool for atomic sculpture…..
The Start:The Start:
Xe atoms on a gold surface:
1) shove into place using the STM tip
2) image your art using the same tip
EiglerEigler et al. , IBM et al. , IBM AlmadenAlmaden
EiglerEigler & Schweitzer& SchweitzerNature Nature 344344, 524 (1990) , 524 (1990)
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Quantum corralsQuantum corrals
Remember:Remember:even in 'topology' mode, STM
measures electronic states, notatomic positions
CrommieCrommie, Lutz, , Lutz, EiglerEigler, IBM , IBM AlmadenAlmaden
First build up the fenceFirst build up the fence
….. here Fe on Cu[111]….. here Fe on Cu[111]
Then see what's inside the corral…Then see what's inside the corral…
surface state = 2D electron gas
Science 262, 218 (1993)
Physics Today 46 17 (1993)
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
16
Atomic force microscopyAtomic force microscopy
A tool for nanotechnologyA tool for nanotechnology
Single wall carbon Single wall carbon nantubenantube with a kink with a kink →→SSingle ingle EElectron lectron TTransistorransistor
nownow
future….future….
Dekker group, Delft
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
MFM exampleMFM example
magnetic tip magnetic tip →→ magnetic magnetic constrastconstrast
ferromagnetic domainsferromagnetic domains
after 1 Tesla
amorphous-GdxFe1-x films
ferrimagnetic
Peters & Peters & GoedkoopGoedkoop
CMP-Group, WZI
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
That's all, folks......That's all, folks......
Questions on Spectroscopic methodsQuestions on Spectroscopic methods
1.1. What do we really What do we really measure measure experimentally in a PES experiment ?experimentally in a PES experiment ?
2.2. At what kinetic energy would the midpoint of a Au Fermi edge appAt what kinetic energy would the midpoint of a Au Fermi edge appear in ear in PES with PES with hhνν=38.0 =38.0 eVeV ??
3.3. Where does the surface sensitivity of PES come from ?Where does the surface sensitivity of PES come from ?
4.4. What factors contribute to the width of a feature in a PES experWhat factors contribute to the width of a feature in a PES experiment ?iment ?
5.5. How can we try and see which peaks in a PES spectrum come from wHow can we try and see which peaks in a PES spectrum come from which hich element/orbital ?element/orbital ?
6.6. What do we measure experimentally in an IPES experiment ?What do we measure experimentally in an IPES experiment ?
7.7. What is happening (microscopically) in an XAS experiment ? How cWhat is happening (microscopically) in an XAS experiment ? How could we ould we monitor this process ?monitor this process ?
8.8. To reproduce the dotted data of Cox's Fig 2.6 with XAS, which seTo reproduce the dotted data of Cox's Fig 2.6 with XAS, which set of core t of core level excitations should we measure ? Would this work ?level excitations should we measure ? Would this work ?
9.9. What do we measure experimentally in an XES experiment ? How areWhat do we measure experimentally in an XES experiment ? How are XES XES and PES related ? How are they different ?and PES related ? How are they different ?
10.10. How does EXAFS work ? Why not simply do diffraction ?How does EXAFS work ? Why not simply do diffraction ?
Chapter 2: Spectroscopic MethodsChapter 2: Spectroscopic Methods
Stuff to do till coming Monday:Stuff to do till coming Monday:
i) prepare yourself to be able to i) prepare yourself to be able to present answers to the questions present answers to the questions about Ch. 2 at the blackboard at the about Ch. 2 at the blackboard at the start of Monday's lecture start of Monday's lecture
ii) please read chapter 3 before ii) please read chapter 3 before Monday !!Monday !!