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Photoelectron Spectroscopy
Claudia Rödl and Matteo Gatti
Laboratoire des Solides IrradiésEcole Polytechnique, Palaiseau, France
SOLEIL Theory Day, Gif-sur-Yvette
May 6th, 2014
Methods: Starting from First Principles
First-principles calculations
Density-functional
theory (DFT)
Many-body perturbation
theory (MBPT)
Ground state
structural properties
total energies
charge densities
One-particle excitations
band gaps
band structures
densities of states
Two-particle excitations:
optical absorption
excitonic states
loss spectra
Methods: Starting from First Principles
First-principles calculations
Density-functional
theory (DFT)
Many-body perturbation
theory (MBPT)
Ground state
structural properties
total energies
charge densities
One-particle excitations
band gaps
band structures
densities of states
DO
S /
inte
nsity
HSE06HSE06+G0W0
HSE06+GnW0
ExperimentGhijsen et al. (1988)
-20 -15 -10 -5 0 5 10 15energy [eV]
PBE+UPBE+U+G0W0
PBE+U+GnW0
ExperimentGhijsen et al. (1988)
Two-particle excitations:
optical absorption
excitonic states
loss spectra
Methods: Starting from First Principles
First-principles calculations
Density-functional
theory (DFT)
Many-body perturbation
theory (MBPT)
Ground state
structural properties
total energies
charge densities
One-particle excitations
band gaps
band structures
densities of states
DO
S /
inte
nsity
HSE06HSE06+G0W0
HSE06+GnW0
ExperimentGhijsen et al. (1988)
-20 -15 -10 -5 0 5 10 15energy [eV]
PBE+UPBE+U+G0W0
PBE+U+GnW0
ExperimentGhijsen et al. (1988)
Two-particle excitations:
optical absorption
excitonic states
loss spectra
0 10 20 30 40 50 60 70 80 900
0.5
1
1.5
20.1
0.3
0.5
0.7
0.9
energy [eV]
q
Cu 3p statesmain plasmon peak
plasmons
ETSF Photoemission Beamline
Systems:
insulators
semiconductors
metals
correlated oxides
Codes:
Dimensions:
bulk
surfaces
molecules
nanosystems
up to ∼ 100 atoms
ETSF Photoemission Beamline
Simulating photoemission
Spectral function Beyond spectral function
Quasiparticle (QP)
approximation:
QP band structures
QP band gaps
DOS
GW method
Beyond QPs:
lifetimes
satellites
(e.g. plasmon
satellites)
GW method
cumulant expansion
Towards reality:
matrix-element effects
(photoionization
cross-sections)
extrinsic and
interference effects
background
Photoemission and the Many-Body Problem
probe the electronic structure
E(N)0 + Eph = E
(N−1)n + Ekin + Φ
Eph = E(N−1)n − E
(N)0
︸ ︷︷ ︸
EB
+Ekin + Φ
Photoemission and the Many-Body Problem
probe the electronic structure
E(N)0 + Eph = E
(N−1)n + Ekin + Φ
Eph = E(N−1)n − E
(N)0
︸ ︷︷ ︸
EB
+Ekin + Φ
EVBM ECBM
DO
S
EFEvac
EB φ
Eph
Ekin
Photoemission and the Many-Body Problem
probe the electronic structure
E(N)0 + Eph = E
(N−1)n + Ekin + Φ
Eph = E(N−1)n − E
(N)0
︸ ︷︷ ︸
EB
+Ekin + Φ
EVBM ECBM
DO
S
EFEvac
EB φ
Eph
Ekin
Ekin
inte
nsity DOS
DOS weighted bycross sections
background
Photoemission and the Many-Body Problem
probe the electronic structure
E(N)0 + Eph = E
(N−1)n + Ekin + Φ
Eph = E(N−1)n − E
(N)0
︸ ︷︷ ︸
EB
+Ekin + Φ
EVBM ECBM
DO
S
EFEvac
EB φ
Eph
Ekin
Ekin
inte
nsity DOS
DOS weighted bycross sections
background
requires full solution of the interacting many-body problem: E(N)0 , E
(N−1)n
Key Quantity: Green’s Function
Green’s function: G(r1t1, r2t2) =1i~
〈N| T ψ(r1t1)ψ+(r2t2) |N〉
Key Quantity: Green’s Function
Green’s function: G(r1t1, r2t2) =1i~
〈N| T ψ(r1t1)ψ+(r2t2) |N〉
Electron propagator:
〈N|ψ(r1t1)ψ+(r2t2) |N〉
electron addition
inverse photoemission
Key Quantity: Green’s Function
Green’s function: G(r1t1, r2t2) =1i~
〈N| T ψ(r1t1)ψ+(r2t2) |N〉
Electron propagator:
〈N|ψ(r1t1)ψ+(r2t2) |N〉
electron addition
inverse photoemission
Hole propagator:
〈N|ψ+(r2t2)ψ(r1t1) |N〉
electron removal
photoemission
Spectral Function and Quasiparticles
real space reciprocal space
Spectral function: A(ω) = Tr |Im G(ω)|
Density of states: DOS(ω) ∼ A(ω)sp
ectr
al fu
nctio
n-20 -15 -10 -5 0
energy [eV]
inte
nsity
weak correlations
non-interacting particles
strong correlations
weak satellite
dominating satellite
QP peak
CuO photoemission
Experimental data:Ghijsen et al., PRB 38, 11322 (1988)
Spectral Function and Quasiparticles
real space reciprocal space
Spectral function: A(ω) = Tr |Im G(ω)|
Density of states: DOS(ω) ∼ A(ω)sp
ectr
al fu
nctio
n-20 -15 -10 -5 0
energy [eV]
inte
nsity
weak correlations
non-interacting particles
strong correlations
weak satellite
dominating satellite
QP peak
CuO photoemission
Experimental data:Ghijsen et al., PRB 38, 11322 (1988)
Spectral Function and Quasiparticles
real space reciprocal space
Spectral function: A(ω) = Tr |Im G(ω)|
Density of states: DOS(ω) ∼ A(ω)sp
ectr
al fu
nctio
n-20 -15 -10 -5 0
energy [eV]
inte
nsity
weak correlations
non-interacting particles
strong correlations
weak satellite
dominating satellite
QP peak
CuO photoemission
Experimental data:Ghijsen et al., PRB 38, 11322 (1988)
ETSF Photoemission Beamline
Simulating photoemission
Spectral function Beyond spectral function
Quasiparticle (QP)
approximation:
QP band structures
QP band gaps
DOS
GW method
Beyond QPs:
lifetimes
satellites
(e.g. plasmon
satellites)
GW method
cumulant expansion
Towards reality:
matrix-element effects
(photoionization
cross-sections)
extrinsic and
interference effects
background
Density-Functional Theory (DFT)
Kohn-Sham equations: Kohn, Sham, Phys. Rev. 140, A1133 (1965)[
−~
2
2m0
∆+ Vext(r) + VH(r, [n]) + VXC(r, [n])
]
ϕnk(r) = εnk ϕnk(r)
density: n(r) =
occ∑
nk
|ϕnk(r)|2
self-consistent solution
Density-Functional Theory (DFT)
Kohn-Sham equations: Kohn, Sham, Phys. Rev. 140, A1133 (1965)[
−~
2
2m0
∆+ Vext(r) + VH(r, [n]) + VXC(r, [n])
]
ϕnk(r) = εnk ϕnk(r)
density: n(r) =
occ∑
nk
|ϕnk(r)|2
self-consistent solution
Exchange-correlation potential VXC?
local potential VXC(r, [n]): LDA, PBE, ...
non-local potential VXC(rr′, [n]):
hybrid functionals (PBE0, HSE06, ...)
on-site term U for localized orbitals (LDA+U, ...)
Density-Functional Theory (DFT)
Kohn-Sham equations: Kohn, Sham, Phys. Rev. 140, A1133 (1965)[
−~
2
2m0
∆+ Vext(r) + VH(r, [n]) + VXC(r, [n])
]
ϕnk(r) = εnk ϕnk(r)
density: n(r) =
occ∑
nk
|ϕnk(r)|2
self-consistent solution
Problems:
Kohn-Sham band structure has no physical meaning (strictly speaking)
band-gap problem: strong underestimation of band gaps
electron addition and removal properties wrong
adapted from M. van Schilfgaarde et al., PRL 96 (2006)
Why more than DFT?
LDA = “band theory” ?
Fujimori et al, PRL 69 (1992)
Why more than DFT?
Quasiparticle Excitations
Quasiparticle Excitations
Quasiparticle Excitations
Quasiparticle equation:[
−~
2
2m0
∆+ Vext(r) + VH(r)
]
ϕnk(r) +
∫
dr′ Σ(r r
′, ω = εnk/~)ϕnk(r′) = εnk ϕnk(r)
Problems:
exchange and correlation: non-local and frequency-dependent self-energy Σ
self-consistent solution
no explicit expression for the self-energy
Hedin’s GW Approximation
Self-energy: Σ ≈ i~G W
Green’s function G(r1t1, r2t2)
Hedin, Phys. Rev. 139, A796 (1965)
Hedin, Lundqvist, Solid State Phys. 23, 1 (1969)
Dynamically screened
Coulomb interaction W (r1r2, ω)
Hedin’s GW Approximation
Self-energy: Σ ≈ i~G W
Green’s function G(r1t1, r2t2)
Electron propag.: 〈N|ψ(r1t1)ψ+(r2t2) |N〉
Hole propag.: 〈N|ψ+(r2t2)ψ(r1t1) |N〉
Hedin, Phys. Rev. 139, A796 (1965)
Hedin, Lundqvist, Solid State Phys. 23, 1 (1969)
Dynamically screened
Coulomb interaction W (r1r2, ω)
Hedin’s GW Approximation
Self-energy: Σ ≈ i~G W
Green’s function G(r1t1, r2t2)
Electron propag.: 〈N|ψ(r1t1)ψ+(r2t2) |N〉
Hole propag.: 〈N|ψ+(r2t2)ψ(r1t1) |N〉
Hedin, Phys. Rev. 139, A796 (1965)
Hedin, Lundqvist, Solid State Phys. 23, 1 (1969)
Dynamically screened
Coulomb interaction W (r1r2, ω)
W (r1r2, ω) =∫
dr3 ε−1(r1r3, ω) v(r3 − r2)
Hedin’s GW Approximation
Self-energy: Σ ≈ i~G W
Green’s function G(r1t1, r2t2)
Electron propag.: 〈N|ψ(r1t1)ψ+(r2t2) |N〉
Hole propag.: 〈N|ψ+(r2t2)ψ(r1t1) |N〉
Hedin, Phys. Rev. 139, A796 (1965)
Hedin, Lundqvist, Solid State Phys. 23, 1 (1969)
Dynamically screened
Coulomb interaction W (r1r2, ω)
W (r1r2, ω) =∫
dr3 ε−1(r1r3, ω) v(r3 − r2)
main contribution:
dynamical screened exchange(Hartree-Fock: ε−1(r1r3, ω) ≡ 1)
adapted from M. van Schilfgaarde et al., PRL 96 (2006)
Why more than DFT?
Fujimori et al, PRL 69 (1992)
LDA = “band theory” ?
Also missing physics!
Mott insulators?
Fujimori et al, PRL 69 (1992)
Exchange + Correlation
LDA = “band theory” ?
Also missing physics!
The role of nonlocal exchange
F. Iori, M. Gatti and A. Rubio, PRB 85 (2012)Exp. from H. Roth PhD thesis – Köln 2008
Bin
din
g e
ner
gy
ARPES vs. band structure: ZnO
Exp from M. Kobayashi, et al. Proceedings of the 29th International Conference on the Physics of Semiconductors (2008)André Schleife PhD thesis, University of Jena (2010)
ETSF Photoemission Beamline
Simulating photoemission
Spectral function Beyond spectral function
Quasiparticle (QP)
approximation:
QP band structures
QP band gaps
DOS
GW method
Beyond QPs:
lifetimes
satellites
(e.g. plasmon
satellites)
GW method
cumulant expansion
Towards reality:
matrix-element effects
(photoionization
cross-sections)
extrinsic and
interference effects
background
Electron Correlation ... 3-Particle Problem
Romaniello et al., PRB 85, 155131 (2012)
Electron Correlation ... 3-Particle Problem
Σ = i~GW
plasmon satellite series
Langreth, PRB 1, 471 (1970)
Aryasetiawan et al.,
PRL 77, 2268 (1996)
Guzzo et al.,
PRL 107, 166401 (2011)
Romaniello et al., PRB 85, 155131 (2012)
Electron Correlation ... 3-Particle Problem
Σ = i~GW
plasmon satellite series
Langreth, PRB 1, 471 (1970)
Aryasetiawan et al.,
PRL 77, 2268 (1996)
Guzzo et al.,
PRL 107, 166401 (2011)
Σ = i~GT
hole-hole or electron-hole
T matrix
6 eV satellite in NiSpringer et al., PRL 80, 2389 (1998)
Romaniello et al., PRB 85, 155131 (2012)
Spectral Function ... Plasmon Satellites
CuO
-20 -15 -10 -5 0 5energy [eV]
00.10.20.30.40.50.60.70.80.9
11.11.21.31.41.51.61.7
- Im
ε-1
(ω)
/ XP
S [a
rb. u
.]
Cu 2p1/2
Cu 2p3/2
valence
valence
EELS
satellite QP
XPS
satellite: response of the material
to the photoemission hole
remaining in the system
plasmon excitations
prominent loss peaks shouldappear in satellite structure
Experimental data:Siemons, PhD thesis (2008)Ghijsen et al., PRB 38, 11322 (1988)Shen et al., PRB 42, 8081 (1990)
Fujimori et al, PRL 69 (1992)
Correlated metals:Satellites?
Adding/removing electrons: reaction of all the others
Correlation = coupling of excitations
Quasiparticle Plasmons(waves of charge)
Metal-Insulator transition in VO2
Dynamical correlation: VO2
M. Gatti, G. Panaccione, and L. Reining (submitted)Spectral function
-Im ε-1(q,ω)
W(r,r',ω) = ε-1(r,r',ω)v(|r-r'|)
Metal-Insulator transition in VO2IXS/EELS
Spectral function
Dynamical correlation: VO2
Metal-Insulator transition in VO2
Spectral function
IXS/EELS-Im ε-1(q,ω)
W(r,r',ω) = ε-1(r,r',ω)v(|r-r'|)
Dynamical correlation: VO2
Ralf Hambach, PhD thesis, Ecole Polytechnique (2010)
Dynamical correlation: VO2
See Francesco's talk
ETSF Photoemission Beamline
Simulating photoemission
Spectral function Beyond spectral function
Quasiparticle (QP)
approximation:
QP band structures
QP band gaps
DOS
GW method
Beyond QPs:
lifetimes
satellites
(e.g. plasmon
satellites)
GW method
cumulant expansion
Towards reality:
matrix-element effects
(photoionization
cross-sections)
extrinsic and
interference effects
background
hν
hν
Matrixelements
Background
Interference &Extrinsic effects
TCOs: Including Photoionization Cross-Sections
ZnO
-25 -20 -15 -10 -5 0 5 10 15 20
DO
S (a
rb. u
.)
-10 -8 -6 -4 -2 0 2
TheoryExp.
-30 -25 -20 -15 -10 -5 0Energy (eV)
-6 -4 -2 0 2
Phot
oem
issi
on in
tens
ity (
arb.
u.)
Zn 4sO 2s Zn 4pO 2ptotal
Zn 3d
UPS (21.2 eV)
XPS (1486.6 eV)
(a) ZnO
SnO2
-30 -25 -20 -15 -10 -5 0 5 10 15 20
DO
S (a
rb. u
.)
-10 -8 -6 -4 -2 0 2
TheoryExp.
-28 -24 -20 -16 -12 -8 -4 0Energy (eV)
-12 -10 -8 -6 -4 -2 0 2Ph
otoe
mis
sion
inte
nsity
(ar
b. u
.)
Sn 5sO 2s
Sn 5pO 2p
total
Sn 4d
UPS (40 eV)
XPS (1486.6 eV)
(c) SnO2
Rödl et al., Phys. Stat. Solidi A 211, 74 (2014)
Matrix elements: V2O
3
E. Papalazarou, et al., PRB 80 (2009)
Getting closer to what is really measured
Spectral function
Getting closer to what is really measured
+ Background
Getting closer to what is really measured
+ Matrix elements
Getting closer to what is really measured
+ Interference/extrinsic effects
Valencebands
Satellites
M. Guzzo, et al, PRL 107 (2011)
Valencebands
Satellites
Spectral function Photocurrent
Getting closer to what is really measured
Adding/removing electrons: reaction of all the others
Correlation = coupling of excitations
Quasiparticle Plasmons(waves of charge)
Adding/removing electrons: reaction of all the others
Correlation = coupling of excitations
Quasiparticle Plasmons(waves of charge)
ExcitonsOrbitonsMagnonsPhonons
…
More couplings...
Springer, Aryasetiawan, Karlsson, PRL 80, 2389 (1998)
6 eV satellite in Ni: 2-hole bound state
Outlook: coupling with other excitations
Back up slides
Interacting particles
Interacting particles
Interacting particles
Probing Neutral Electronic Excitations
Inelastic scattering of
Electrons
electron-energyloss spectro-
scopy (EELS)
low q
X-rays
non-resonant
inelastic x-rayscattering (IXS)
large q
charge density fluctuations (interband transitions, excitons, plasmons)
charge-density response function χ(r1r2, t1 − t2)
χ(r1r2, t1 − t2) =1i~〈N| T ∆n(r1, t1)∆n(r2, t2) |N〉
Probing Neutral Electronic Excitations
Inelastic scattering of
Electrons
electron-energyloss spectro-
scopy (EELS)
low q
X-rays
non-resonant
inelastic x-rayscattering (IXS)
large q
charge density fluctuations (interband transitions, excitons, plasmons)
charge-density response function χ(r1r2, t1 − t2)
χ(r1r2, t1 − t2) =1i~〈N| T ∆n(r1, t1)∆n(r2, t2) |N〉
loss function − Im ε−1(q, ω)
ε−1(q, ω) = 1 + v(q)χ(qq, ω)
Probing Neutral Electronic Excitations
Inelastic scattering of
Electrons
electron-energyloss spectro-
scopy (EELS)
low q
X-rays
non-resonant
inelastic x-rayscattering (IXS)
large q
charge density fluctuations (interband transitions, excitons, plasmons)
charge-density response function χ(r1r2, t1 − t2)
χ(r1r2, t1 − t2) =1i~〈N| T ∆n(r1, t1)∆n(r2, t2) |N〉
loss function − Im ε−1(q, ω)
ε−1(q, ω) = 1 + v(q)χ(qq, ω)
dynamic structure factor S(q, ω)
S(q, ω) ∼ χ(qq, ω)