introduction to x-ray spectroscopypages.cnpem.br/synclight2015/wp-content/uploads/sites/46/...energy...
TRANSCRIPT
Introduction to X-ray
Spectroscopy
Pieter Glatzel
Books
J. J. Sakurai:
“Advanced Quantum Mechanics”
Addison Wesley, 1967
G. Bunker:
“Introduction to XAFS”
Cambridge Press, 2010
F.M.F. de Groot and A. Kotani:
“Core level spectroscopy of solids”
Taylor and Francis, 2008
W. Schülke:
“Electron Dynamics by Inelastic X-ray
Scattering”
Oxford University Press, 2007
Michel van Veenendaal:
“Theory of Inelastic Scattering and
Absorption of X-rays”
Cambridge University Press, 2015
Reminder: The photon
hchE
Energy
0 100 000 eV5 eV 100 eV 1000 eV1 eV
4
Linear momentum
2, kkp
Photon intrinsic angular momentum
5Wikipedia
Energy
0 100 000 eV
Infrared
VUV
Raman
Soft X-ray Hard X-rayUV-Vis
5 eV 100 eV 1000 eV1 eV
Vibration
Valence shell Core levels
The response of the system that is probed by photons
depends on the photon energy.
6
Spectroscopy
What may happen in the sample?
h
1s
3d
EF
A single electron energy diagram is simple and qualitative.
A simplified view: An electron is excited to an unoccupied orbital.
2p
Electronic and atomic structural information
Element specific
Bulk sensitive; compatible with
in-situ and extreme conditions
XAS XES
Why X-ray Spectroscopy
Soft X-Rays Hard X-Rays
Soft and hard X-rays to study electronic structure
Tender X-rays
Ideal for electronic structure studies Ideal for in situ studies
Improve in situ conditions Develop new techniques to study electronic structures
L- and K-edges in 3d transition metals
10 Gilbert et al., J. Phys. Chem. A, Vol. 107, No. 16, 2003
2p → 3d 1s → np
Soft X-rays Hard X-rays
Why X-ray spectroscopy?
11
Spectroscopy does not require long range order.
Ideal tool for e.g. catalysis, environmental sciences, biology, …
Identify Cr(V)…
J. Bagar et al., SSRL
Electromagnetic radiation
trkieAA
ˆ0
Interaction of X-rays with matter
Describe photon with vector field:
q
q: scattering angle
kin-kout=q (momentum transfer)
in-out (energy transfer)
q
In first order, a term in
A2 is retained.
In second order, a term in
A∙p is retained.
A
)ˆ,,( outoutout k
)ˆ,,( ininin k
Perturbation Theory
Perturbation Theory: Two scattering terms
2A
Ap
)ˆ,,( ininin k
)ˆ,,( outoutout k
n
The A2 term and the dynamic structure factor
Thomson scattering: in=out
Bragg scattering: in=out
Raman scattering: out<in
Compton Scattering: out<in
q
with
outin
i
rqikkqeO i
;ˆ
)ˆ,,( outoutout k
)ˆ,,( ininin k
Dynamic Structure Factor
f
outingfoutin
in
outoutin EEgOfF
2* ˆ),(
THE RESONANT SCATTERING TERM: XES, RXES, RIXS, RXRS, HERFD
Perturbation Theory: Two scattering terms
2A
Ap
)ˆ,,( ininin k
)ˆ,,( outoutout k
n
The A∙p term
(resonant) X-ray emission
(RXES, RIXS, fluorescence, XAS)
q
Kramers and Heisenberg
f
outingf
n ningnin
outoutin
KH EEiEE
gOnnOfF
2† ˆˆ
),(
)ˆ,,( outoutout k
)ˆ,,( ininin k
...))(ˆ(ˆ
ˆ
rkrr
epOj
rki
jj
1s13dn+1
3p53dn+1
1s13dnp
3p53dnp
Tota
l En
ergy Kb
EF
1s
2p
3p
3d3d
nKb rKb
One-electron diagram Many body diagram
Transition schemes
1s23dn
Energy scheme and spectroscopy
Total
Energy
FeIII [Ar 3d5]
1s13d5(p)1
2p53d5(p)1
1s13d6
3d6MOn-1
|g>
|<n|Ô|g>|2
in
2p53d6
3p53d5(p)1
3p53d6
M-edge
Ka
Kb
Valence-to-core
UV-Vis
L-edge
out
|n>
HEtotalˆ
Single crystal
monochromator
Ei, I0
Sample
Ei, I1
Ee, I21
0ln)(I
IEi
2)( IEi
Photon-in/photon out spectroscopy
Fluorescence
Single crystal
monochromator
Ei, I0
Sample
Ei, I1
Ee, I2
Analyzer crystal
1
0ln)(I
IEi
X-ray Emission
Photon-in/photon-out spectroscopy
Fluorescence
2)( IEi
ESRF ID26
)ˆ,,( outoutout k
)ˆ,,( ininin k
What can inner-shell spectroscopy do?
Inner-shell spectroscopy probes electronic transitions and thus the electron
density or electron configuration. This may tell you about:
• The chemical environment
o bond distances
o bond angles
o type and number of ligands
• The spin-orbit term of the ground state: The measured spectrum represents
excited states that are linked to the ground state via the transition matrix
element. The transition probability depends on the ground state symmetry,
e.g. the spin state, formal oxidation state
|g>
|n>
1S
1P2S+1L
DS=0
DL=0;±1
What is oxidation state: Atoms and electron density
When “measuring” oxidation state we often ask “what is the charge per atom?”
2r(r) and MO in a Ni complex
Is that the right question to ask?
The idea of an atom
Wikipedia:
“Noumenon: An object knowable by the mind or intellect, not by the senses;”
… a noumenon in the sense of Kant.
… an experimentalist has no doubt that he or
she is measuring the properties of a single
atom…
Orbital relaxation
All electrons will adjust after excitation with X-rays:
Always consider ALL electrons when describing the energy levels.
The potential experienced by all electrons changes after photoexcitation.
Two-electron excitation
Valence Orbital
Empty Orbital
The orbitals may adjust non-adiabatically, i.e. electrons are excited to higher orbitals
upon orbital relaxation (additionally to the electron that is photo-excited).
The inner-shell absorption proces
Energy
g
n
T lcaabs OSgOn r 2
2
0
2
Many-electron
wavefunction
One-electron
wavefunction
≈ 3d6
≈ 1s13d64p1
≈ 1s → 4p
h
Approximate multi-
electron effects by
scaling factor S02
Electronic structure calculations and inner-shell spectroscopy
Ligand field multiplet theory
Start with ion in spherical symmetry
Branch to real symmetry
Include covalency using
configuration interaction (CI)
Good treatment of core hole effect
and multi-electron excitation
Electron density calculations
Start with structure
Include core hole
Include multi-electron excitations
Good treatment of ligands/long
range order
1
N!
1(r
1 ) 1( r
2 ) 1(r
N )
2( r
1)
N ( r
1 ) N ( r
N )
empirical
approximative
(e.g. to Oh)
Multi-electron excitations
Multi-electron
excitation
Experiment: Ce L3 (2p3/2) edge
One-electron calculationSingle impurity Anderson model
~f0~f1
No multi-electron excitations
Correct crystal field splitting
Multi-electron excitations
Empirical crystal field splitting
EXPERIMENTAL ARTEFACTS
Secondary process detection
t
dA
XESA
eEKII
t
1
sin
)(0
sin
)(
sin
)( Fttt
EEA
lsdscsfsfJK
4
J jumping ratio – PE of shell of interest
fluorescence yield per shell
f fractional yield per subshell
fs fraction of line measured with spectrometer
cs crystal efficiency
ds detector efficiency
ls losses due to absorption (windows, beam path in air)
The goal is to determine (E) by recording the intensity of the scattered X-rays
Selective fluorescence detection in CoFe2O4
Total fluorescence
yield
Fe fluorescence
yieldt
dA
XESA
eEKII
t
1
sin
)(0
The total absorption appears in the denominator
TFY and HERFD on CoFe2O4
Total fluorescence
yield
Fe fluorescence
yield
Experiment
Calculation using tabulated values
after edge
before edge
J. Synchrotron Rad. (2012). 19, 911–919
Incident Beam Self Absorption
Incident Beam Self Absorption
compresses the intensity of a
spectrum
Incident beam self absorption (IBSA) arises from a similar mechanism as the
dip seen in the previous slides but for the same element.
36
RADIATION DAMAGE
If a leaf can do it, we can do it too!
Lubitz and Messinger, Energy and Environmental Science, 2008
Photosynthesis
The Sample
Spinacia oleracea
Photosystem IIMulti-protein complex Photosystem-II
Damage of the Mn cluster
41
6540 6550 6560 6570Incident Energy [eV]
Dealing with radiation sensitive samples on ID26
Page 42
Spectral change at fixed energy as function of time.
beam size: 700 x 100 m; ~2*1013 photons/second
Dealing with radiation sensitive samples
l Title of Presentation l Date of Presentation l AuthorPage 43
Each energy point measured in
different position of beam on
sample.
Take map of metal
fluorescence response.
Science 316, 1444-1448 (2007); Nature 406, 752-757 (2000)
Detect and Destroy at a free electron laser
Kern et al. Science 340 (2012) 491
PSII and the free electron Laser
XFEL provides correct Kb spectra
Kern et al. Science 340 (2012) 491
1s
2p
3p
VS
THE ENERGY LEVELS OF LOCALIZED ORBITALS
3d orbitals in a crystal field
48
10Dq
atomict2g
eg
Oh
Octahedral and tetrahedral coordination
49
ChemWiki @ UC Davis
3d orbitals in a crystal field
50
ChemWiki @ UC Davis
MULTIPLET THEORY
An open shell
Et = Erest + E3d
Et =Erest + ?
How can we treat open shells ? → MULTIPLET THEORY
3d orbitals
Treating electron-electron interactions
j>i
j>i
ij
ji|g|ijij|g|ij
|g|
"direct term" > 0 "exchange term" > 0
Matrix element for two-electron operator:
“Slater integrals or Racah parameters”
gijj1
i1
g( ri
i j
i 2
N
, rj
)two-electron operator:
An open shell: 3d2
40
221
2121
21
L
ll
llllL
llL
The Racah parameters determine the magnitude of the splitting.
Angular momentum coupling
(Total Angular Momentum)
(for d-electrons)
(S,P,D,F,G)
d2
3F
1D3P
1G
1S
Notation: 2S+1L
Crystal Field Splitting: Tanabe-Sugano diagram
Atom Oh coordination
Additional splitting due to orbital hybridization (ligand field theory)
→ The spectra become very very complex already for d2
d2
3d
t2g
eg
Inner-shell spectra are often very complex
56
Intra-valence shell electron-electron interactions
Core hole – valence electron interactions
Multi-electron excitations
3d5
2p5
RESONANT INELASTIC X-RAY SCATTERING: RIXS, HERFD
Hard X-ray Photon-in/Photon-out spectroscopy
Single crystal
monochromator
Ei, I0
Sample
Ei, I1
Ee, I2
I2~ (Ei)
1
0ln)(I
IEi
Incident Energy (Ei) [eV]
Ee
2p
3d
4f5d
Ei
2p
3d
4f5d
Second order process
Correctly treated with
Kramers-Heisenberg equation
CeO2
L3-edge
Hard X-ray Photon-in/Photon-out spectroscopy
Single crystal
monochromator
Ei, I0
Sample
Ei, I1
Ee, I2
Ee
2p
3d
4f5d
I2~ (Ei)
1
0ln)(I
IEi
Incident Energy (Ei) [eV]
Analyzer crystal
Energy Transfer (Ei-Ee) [eV]
XES
Ei
2p
3d
4f5d
XAS
Hard X-ray Photon-in/Photon-out spectroscopy
Single crystal
monochromator
Ei, I0
Sample
Ei, I1
Ee, I2
I2~ (Ei)
1
0ln)(I
IEi
Incident Energy (Ei) [eV]
Analyzer crystal
Energy Transfer (Ei-Ee) [eV]
XAS
CeO2 XAS
TFY
HERFD
Conventional TFY
High resolution XANES
CeO2 XAS
Conventional TFY
High resolution
(HERFD-XAS)
Fine structure of 5d band
4f
5d
Resolve fine structure in 5d band (crystal field splitting)
Resolve 4f orbitals
High resolution XANES
2p3d (La) RIXS plane in CeO2
2p3/2 hole
3d
ho
le
• The 3d and 2p core hole potentials are similar.
• Weak interaction of core hole with photoexcited
electron
Spectral features appear along diagonal streak.
Hämäläinen et al., Phys. Rev. Lett. 67 2850 (1991)
Carra et al. PRL 74 3700 (1995)
Glatzel et al., J. Electr. Spectr. Relat. Phenomena 188 (2013) 17-25
Kotani et al., J. Electr. Spectr. Relat. Phenomena 184 (2011) 210–215
z3d
Direct study of the valence shell
Ce 2p → 4f excitations
Kvashnina et al., JAAS 26 1265 (2011)
p
p
2
2
d
d
3
3
Ground State
Intermediate (absorption) State
Final State
Tota
l E
nerg
y
Energy
transfer
Incident Energy
XAS
Emitted Energy
XES
Lifetime broadening and continuum excitations
The RIXS planeTota
l E
nerg
y
Incident Energy
Energ
y T
ransfe
r
Energy
transfer
The RIXS/RXES plane
Incident Energy
Energ
y T
ransfe
r n
fEnerg
y T
ransfe
r
n
f
f
outingf
n ningnin
outoutin
KH EEiEE
gOnnOfF
2† ˆˆ
),(
Simplifying the Kramers-Heisenberg Formula
Ignore Interference and simplify:
f
outingf
n ningnin
outoutin
KH EEEE
gOnnOfF
22
22†
)(
ˆˆ
),(
|g>, Eg
|n>, En
|f>, Ef
in
Interference changes intensities but not energies.
out
Does the scattered photon forget?
f
outingf
n ningnin
outoutin
KH EEiEE
gOnnOfF
2† ˆˆ
),(
Simplifying the Kramers-Heisenberg Formula
Ignore Interference and simplify:
|g>, Eg
|n>, En
|f>, Ef
Interference changes intensities but not energies.
XASXES
f
outingf
n ningnin
outoutin
KH EEEE
gOnnOfF
22
22†
)(
ˆˆ
),(
Tota
l E
nerg
y
Tota
l E
nerg
y
Atomic multiplet model calculations for 4f0
2p54f1 2p54f1
3d94f13d94f1
No 3d – 4f interaction With 3d – 4f interaction
4f0 4f0
4f0
No 3d – 4f interaction With 3d – 4f interaction
Tota
l E
nerg
y
Tota
l E
nerg
y
2p54f2 2p54f2
3d94f23d94f2
4f1 4f1
Atomic multiplet model calculations for 4f1
4f1
Kvashnina et al., JAAS 26 1265 (2011)
No 3d – 4f interaction With 3d – 4f interaction
Tota
l E
nerg
y
Tota
l E
nerg
y
2p54f2 2p54f2
3d94f23d94f2
4f1 4f1
Atomic multiplet model calculations for 4f1
4f1
Kvashnina et al., JAAS 26 1265 (2011)
Interference No Interference
Comparison with Experiment
4f0 4f1
Interference No Interference
Experiment
Theory
Kvashnina et al., JAAS 261265 (2011)
A little history of Ceria
The Relevance of Ceria
The Spectroscopy on Ceria
The Theory applied to Ceria
The Confusion around Ceria
The Defects in Ceria
The Relevance of CeO2
Solid oxide fuel cell
PNAS 2006;103:3495-3496
CeO2 ↔ CeO2- + /2 O2
Labeling of cancerous cells
Have we understood bulk CeO2?
Atomic Structure of Ceria
CeO2
Formally: CeIV 4f0
Cubic
One Ce site
Bulk Ceria during the 80’s
Ce 4f and O 2p mix
4f levels are populated in ground state
n4f ~ 0.5
1983
Homogeneous mixed valence
4f0
Bulk Ceria during the 80’s
3d XPS
Fujimori, PRB 28 2281 (1983)
Homogeneous mixed
valence
Bianconi et al., PRB 35 806 (1987)
4f0
2p3/2 XAS
Bulk Ceria during the 80’s
Wuilloud et al. PRL 53 202
(1984)
« a mixed valence can be
definitely excluded »
Nakano et al. JPSJ 56 2201
(1987)
« The number of 4f electrons is
between 0.36 and 0.54 «
Homogeneous mixed
valence
4f0
4f0
Bulk Ceria in the 21st century
4f0
4f0
RIXS:
Sham et al. Phys Rev B 72, 035113 (2005):
“… CeO2 in the initial state is Ce4+ (4f0) ...”
Hybrid DFT:
Graciani et al. J. Chem. Theory and Comp. 7 56 (2011)
“All valence Ce states, including the 4f states, are empty”
Almost all publications presenting DFT calculations
Bond Valence Method:
Shoko et al. Phys Rev B 79, 134108 (2009):
“… we conclude that CeO2 is a mixed-valent
compound....”
RIXS:
Kvashnina, Kotani, Butorin, Glatzel
J. Electr. Spectr. Relat. Phenomena 184 (2011) 210–215
Sadly, very little new insight over the past 30 years.
Can we determine the charge per atom?
Cococcioni et al. (PRB 71 035105 (2005)) :
“… there is no unique or rigorous way to define occupation of localized atomic levels
in a multiatom system…”
Ce d-DOS
Ce f-DOS
O p-DOS
Metal ionLigand
e-
+ + e-
photoexcitation
Metal ionLigand
Ground State Excited State
e
a
e
b
screened
Non-screened
The Single Impurity Anderson Model
4sin4cos 10 Lffg
b bb
Gunnarsson and Schönhammer, PRB 28 4315 (1983)
e-
Multi-electron excitations in CeO2
~f0
~f1L Total fluorescence yield
High resolution XAS
One-electron calculations
Surface reduction observed using TEM-EELS
Turner et al.,
Nanoscale 3 3385
(2011)
CeO2 on Pt (111) under vacuum
with L. Amidani, F. Pagliuca, F. Boscherini
In-situ study of CeO2 nanoparticle synthesis
10 mM
ACS Nano, 2013, 7 (12), pp 10726–10732
IN-SITU STUDY OF CEO2 NANOPARTICLE SYNTHESIS
5710 5720 5730 5740 5750 5760 5770 5780
5716 5718 5720 5722
Inte
nsity/a
.u
Energy /eV
Inte
nsity/a
.u
Energy /eV
Reaction time/hr
Ce(NO3)3.6H2O
CeO2
Pre-edge
2p → 4f
0 5 10 15 200.0
0.2
0.4
0.6
0.8
1.0
Ce4+
Ce3+
We
ight
fra
nctio
nReaction time/h
Ce(NO3)3
CeO2 NP
60 seconds one scan
ACS Nano, 2013, 7 (12), pp 10726–10732
BLURRING OF 5D BAND STRUCTURE
5.72 5.73 5.74 5.75 5.76
NPs 25 nm
NPs belt
NPs 15 nm
NPs 10 nm
NPs 3.2 nm
No
rma
lize
d in
ten
sity (
a.u
.)
Incident energy (keV)
5d band
3 nm
Paun et al., J. Phys. Chem. C 2012,
116, 7312-7317
Ce ion Ligand
e-
SPIN MULTIPLICITY AND ORBITAL MOMENT
4sin4cos 10 Lffg
b bb
1S
Ce ion Ligand
e-
14 fg
b
2F2S+1L
CeO2 CeO2-
DIRECT STUDY OF THE VALENCE SHELL
1S
2F
Kvashnina et al., JAAS 26 1265 (2011)
THE CE 4F LEVEL IN NANOPARTICLES
5.718 5.720 5.722 5.724 5.726
No
rma
lize
d in
ten
sity (
a.u
.)
Ce(NO3)3
NPs 25 nm
NPs belt
NPs 15 nm
NPs 10 nm
NPs 3.2 nm
Incident energy (keV)
2F
1S
No Ce 2F in nanoparticles → Are they chemically active?
CHEMICAL ACTIVITY: ADDING H2O2
Celardo et al., Nanoscale 3 1411 (2011)
1
2
6 5
4
3
7
Balancing ROS levels
CHEMICAL ACTIVITY: ADDING H2O2
5710 5720 5730 5740 5750 5760
3nm CeO2
25nm CeO2
Inte
nsity/a
.u
Energy/eV
f1L f0
H2O2
0 5 10 15 20
0.48
0.52
0.56
0.60
f-o
ccu
pancy
Time/hrs
4f-
occupancy
3nm, 25 nm
Time/ hrs
“Reduction”0 5 10 15 20 25 30
3.0
3.5
4.0
4.5
5.0
5.5
CeO2NPs (3nm) + H
2O
2
CeO2NPs (3nm)
pH
Days
IS THERE ANY CE3+ 2F ?
Consistent with initial increase of electron density on Ce and subsequent “oxidation”
No observation of Ce3+ 2F
5716 5718 5720 5722
3nm CeO2
25nm CeO2
Inte
nsity/a
.u
Energy/eV
2p – 4f
0 5 10 15 20
0.48
0.52
0.56
0.60
f-occup
ancy
Time/hrs
4f-
occupancy
3nm, 25 nm
Time/ hrs
ACS Nano, 2013, 7 (12), pp 10726–10732
Electron Sponge
Core-to-core RIXS
Ground State
Intermediate (absorption) State
Final State
Tota
l E
nerg
y
Energy transfer
Incident Energy
XAS
Emitted Energy
XES
~900 eV
Core-to-valence RIXS
Ground State
Intermediate (absorption) State
Final State
Tota
l E
nerg
y
Incident Energy
XAS
Emitted Energy
XES
~1 eV
No core hole in the
final state !
Photon-in/photon-out spectroscopic techniques
1s
2p
3p
L, (3d)
3dEF
vtcKb rvtcrKb
Non-resonant Resonant
TS-1
Titanium in Silicalite – TS-1
NH3
DFT calculations
NH3
Exp. Theory
1 2
ChemPhysChem 14, 79-83 (2013)
DFT and vtc XES
E. Gallo and P. Glatzel, Advanced Materials (2014)
VBs MOrMO
1
Ti silicalite
Use Kohn-Sham orbitals:
Application of RIXS: Combine with magnetic circular dichroism
3d TM X-ray Magnetic Circular Dichroism
L-edge MCD is a great success because of sum rules to determine spin and
orbital angular moments.
In situ experiments at the L-edge very challenging or impossible.
Hard X-rays at the K-edge probe the p-DOS → very weak MCD effect
K-edge MCD difficult to interpret (no spin-orbit split edge)
Compatible with in situ experiments
Magnetic circular dichroism
Energy
g
n
B
B
1Dm 1Dm
XMCD arises from removing the
degeneracy with respect to the magnetic
quantum number m by more than kT and
macroscopically orienting the moments.
Different final states are reached
following the selection rules.
Derive sum rules using ligand field
multiplet theory.
The RIXS-MCD Energy Scheme
Magnetite (Fe3+)tetra (Fe3+)octa (Fe2+)octa O4
RIXS-MCD Experimental Setup
The first RIXS-MCD plane
Experiment Theory
M. Sikora, A. Juhin, et al. PRL 105, 037202 (2010)
Constant emission energy scans
CEE
Sharpening of spectral features
(decreased lifetime broadening)
XMCD enhanced by factor of ~10-20
Direct evidence for the existence of an intermediate interdiffusedlayer
APPLICATION OF RIXS-MCD
A. Juhin, A. Lopez Ortega, M. Sikora, …, J. Nogues, under review
Mn MCD signal!
Kb X-RAY EMISSION SPECTROSCOPY (XES)
x 8
x 500
Kb
The K fluorescence lines in 3d transition metals
1s
2p
3p
VS
The exchange interaction
3p
VS
Acts only between
electrons with parallel
spins and lowers the
total Energy
Etotal
Fluorescence
Exchange energy lowers total
energy
For 3d transition metals the strong chemical sensitivity of core levels does
NOT arise from screening!
Mn4+
Mn3+
Chemically sensitive !!
Chemical sensitivity of Kb Emission
Kb1,3
Kb’
MnF2: S=5/2
MnF3: S=2
MnF4: S=3/2
Wang et al. Phys. Rev. B 56, 4553 (1997)
Screening effect very small (unlike Sulfur!!).
(3p,3d) interactions are dominating.
Model systems and multiplet theory
LS
HS
Crystal field
multiplet model
Experiment
Fe2O3 S=5/2
K3Fe(CN)6 S=1/2
K4Fe(CN)6 S=0
Mn-Mg pairs in GaN
Th. Devillers, M. Rovezzi, et al. Scientific Reports 2 722 (2012)
Kb
Th. Devillers, M. Rovezzi, et al. Scientific Reports 2 722 (2012)
Mn-Mg pairs in GaN
(Mn3+)
(Mn4+)
XAS and XES in a layered Mn perovskite
x XANES
The La1-xSr1+xMnO4 series: doping dependence in powders
Kb
Emission Energy [eV]Absorption Energy [eV]
Replace La3+ by Sr2+ Formally: Mn3+ → Mn3.5+
Linear Dichroism in XES
Single crystal
monochromator
Ei, I0
SampleEi, I1
Ee, I2
e
Single crystal
monochromator
Ei, I0
SampleEi, I1
Ee, I2
e
VALENCE-TO-CORE X-RAY EMISSION SPECTROSCOPY (VTC XES)
x 8
Valence-to-Core X-Ray Emission in 3d Transition Metals
x 500
1s
2p
3p
VS
XES and XAS: Complementary Techniques
Occupied
states
Unoccupied
states
Fermi Energy
XES
XAS
Mn(V)N
1s
2p
3p
VSEF
Fine structure of valence-to-core emission lines
M
M
Transitions from:
Ligand 2p
Ligand 2s
ungerade symmetry with
respect to metal centerBergmann et al., Chem. Phys. Lett. 302 119 (1999)
Safonov et al., J. Phys. Chem. B 110 23192 (2006)
Mainly sensitive to orbitals that are centered on ligands.
Degree of ligand protonation
Lassalle-Kaiser et al., Inorg. Chem. 2013, 52, 12915−12922
ID26