excited states and spectroscopy - max planck society
TRANSCRIPT
Experimental photoemission spectrum152
CH,=CH2
CH,-CH3
25 20 15 10
Phot
oem
issi
on sp
ectru
m
Energy [eV]
C2H4
5
DFT eigenvalues
• direct connection of ionization
potentials (IP) to KS-DFT or HF
orbital energies εKS/HFn
• ionization potentials: IPn = −εKS/HFn
• deviation from experiment for valence
states ≈ 3 eV
Figure 1: Energy levels H2O
6
Ionization potentials from DFT and HF eigenvalues
Exercise 1 and 2
• Calculate electron removal energies from KS-DFT and Hartree-Fock
eigenvalues for C2H4 and optionally H2O.
• Compare the results to experiment.
7
The DFT-∆SCF approach
Ionization potentials
IP = Etot(N − 1)− Etot(N)
• more accurate than eigenvalues
• constraints needed for levels other than HOMO and LUMO
• several conceptual problems, e.g., for periodic systems
8
Ionization potentials and affinities from DFT-∆SCF
Exercise 3
Calculate the ionization potential for the HOMO from the ∆SCF
approach
• IPHOMO = Etot(N − 1)− Etot(N)
Optional : Calculate the electron affinity (A) for the LUMO with ∆SCF
• ALUMO = Etot(N)− Etot(N + 1)
Compare the IPs to the experiment and the DFT and HF eigenvalues.
9
Quasiparticle energies from GW
Basic idea
• in analogy to DFT: replacement of XC potential by self-energy
• self-energy
Σ(r, r′, ω) =i
2π
∫dω′G(r, r′, ω + ω′)W (r, r′, ω′) eiω
′η
• G : Green’s function; W : screened Coulomb interaction
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The G0W0 approach
Single-shot perturbation: G0W0
• correction to KS-DFT orbital energies εKSn
εG0W0n = εKSn + 〈ψKS
n |Σ(εG0W0n )− vxc |ψKS
n 〉• self-energy
Σ(r, r′, ω) =i
2π
∫dω′G0(r, r′, ω + ω′)W0(r, r′, ω′) eiω
′η
Procedure:
1. run DFT calculation
2. calculate G0 and W0 from DFT orbital energies εKSn and MOs {ψKSn }
3. calculate self-energy from G0 and W0
4. solve quasi-particle equation
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The G0W0 approach
Single-shot perturbation: G0W0
• correction to KS-DFT orbital energies εKSn
εG0W0n = εKSn + 〈ψKS
n |Σ(εG0W0n )− vxc |ψKS
n 〉• self-energy
Σ(r, r′, ω) =i
2π
∫dω′G0(r, r′, ω + ω′)W0(r, r′, ω′) eiω
′η
Procedure:
1. run DFT calculation
2. calculate G0 and W0 from DFT orbital energies εKSn and MOs {ψKSn }
3. calculate self-energy from G0 and W0
4. solve quasi-particle equation
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The G0W0 approach
Non-interacting KS Green’s function G0
G0(r, r′, ω) =∑m
ψKSm (r)ψKS
m (r′)
ω − εKSm − iη sgn(εF − εKSm )
Screened Coulomb interaction W0
W0(r, r′, ω) =
∫dr′′ε−1(r, r′′, ω)v(r′′, r′),
with
ε(r, r′, ω) = δ(r, r′)−∫
dr′′v(r, r′′)P0(r′′, r′, ω)
ε ... dielectric function
P0 ... polarizability
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The G0W0 approach
Non-interacting KS Green’s function G0
G0(r, r′, ω) =∑m
ψKSm (r)ψKS
m (r′)
ω − εKSm − iη sgn(εF − εKSm )
Screened Coulomb interaction W0
W0(r, r′, ω) =
∫dr′′ε−1(r, r′′, ω)v(r′′, r′),
with
ε(r, r′, ω) = δ(r, r′)−∫
dr′′v(r, r′′)P0(r′′, r′, ω)
ε ... dielectric function
P0 ... polarizability
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G0W0 output with FHI-aims
State index
Occupation number
Figure 2: Output for the hydrogen molecule
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Ionization potentials from G0W0
Exercise 4.1
Calculate IPs for HOMO, HOMO-1, HOMO-2 and HOMO-3 levels with
the G0W0 approach starting from PBE. Compare the results to
experiment and the previous calculations
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G0W0 basis set convergence
Green’s function G0
G0(r, r′, ω) =all states∑
m
ψKSm (r)ψKS
m (r′)
ω − εKSm − iη sgn(εF − εKSm )
Polarizability P0
P0(r, r′, ω) =occ∑i
virt∑a
ψKSa (r′)ψKS
i (r′)ψKSi (r)ψKS
a (r)
×{
1
ω − (εKSa − εKSi ) + iη+
1
−ω − (εKSa − εKSi ) + iη
}.
Slow convergence!!!
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G0W0 basis set convergence
Exercise 4.2
Test the basis set convergence of G0W0 using basis sets of increasing
size.
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G0W0 starting point dependence
• “Screening”: eigenvalue difference in polarizability:
P0(r, r′, ω) =occ∑i
virt∑a
ψKSa (r′)ψKS
i (r′)ψKSi (r)ψKS
a (r)
×
{1
ω − (εKSa − εKSi ) + iη+
1
−ω − (εKSa − εKSi ) + iη
}.
• “Self-interaction”: directly from DFT eigenvalues:
εG0W0n = εKSn + 〈ψKS
n |Σ(εG0W0n )− vxc |ψKS
n 〉
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G0W0 starting point dependence
• “Screening”: eigenvalue difference in polarizability:
P0(r, r′, ω) =occ∑i
virt∑a
ψKSa (r′)ψKS
i (r′)ψKSi (r)ψKS
a (r)
×
{1
ω − (εKSa − εKSi ) + iη+
1
−ω − (εKSa − εKSi ) + iη
}.
• “Self-interaction”: directly from DFT eigenvalues:
εG0W0n = εKSn + 〈ψKS
n |Σ(εG0W0n )− vxc |ψKS
n 〉
18
G0W0 starting point dependence
Exercise 4.3 and 4.4
Test the starting point dependence of G0W0 with different functionals
for the underlying DFT calculations. Visualize the G0W0 spectra and
compare to the experimental photoemission spectrum of ethylene.
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Self-interaction error for naphthalene
Exercise 6
Compare the energetic ordering of the DFT orbitals and the G0W0
quasiparticle energies for naphthalene. Assess the self-interaction error.
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Self-consistent GW - Spectral function
Spectral function
A(ω) = − 1
π
∫dr lim
r′→rImG (r, r′, ω) sgn(ω − εF )
• fully interacting G from self-consistent GW calculation
• poles of G correspond to excitations
• peaks in A are the excitation energies
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Self-consistent GW
Exercise 5
Perform self-consistent GW for ethylene
• Compute the spectral functions and extract the quasiparticle
energies
• Test the starting point dependence of self-consistent GW
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GW total energy
Galitskii-Migdal equation
EGM = −i∫
dω
2πTr {[ω + h0]G (ω)}+ Eion,
h0 ... single particle term
. V. Galitskii and A. Migdal, Sov. Phys. JETP 7, 96 (1958)
. G from self-consistent GW
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GW total energies
Exercise 7
Calculate the binding energy curve of H2 in self-consistent GW and
compare to full-CI.
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