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Green’s function theory for solid state
electronic band structure
Hong JiangCollege of Chemistry, Peking University
Outline
Introduction: what is Green’s functions for?
Green’s function for single-electron Schrödinger Equations
Green’s function for many-body systems: general formalism
GW approximation and implementation
Applications of the GW approach: examples
Further ReadingsThe GW approach
G. Onida, L. Reining and A. Rubio, Rev. Mod. Phys. 74, 601 (2002).
W. G . Aulbur, L. Jonsson, J. Wilken, Solid State Phys., 54, 1 (2000).
F. Aryasetiawan and O. Gunnarsson, Rep. Prog. Phys. 61, 237 (1998)
L. Hedin and S. Lundqvist, Solid State Phys. 23, 1-181 (1970).
Many-body theory in general
J. C. Inkson, Many-Body Theory of Solids: An Introduction (Plenum Press, 1984).
A. L. Fetter and J. D. Walecka, Quantum Theory of Many-Particle Systems (Dover, 2003).
E. K. U. Gross, E. Runge, O. Heinonen, Many-Particle Theory, (IOP Publishing, 1991).
R. D. Mattuck, A guide to Feynman diagrams in the many-body problem, (McGrow Hill, 1976).
E. N. Economou, Green’s functions in Quantum Physics (3rd ed., Springer, 2006).
Introduction: What are Green’s functions for?
Why are electronic band structure important?
R. M. Navarro Yerga et al. (2009)
Graetzel, Nature (2001)
Electron excitations: experimental measurements
[Yu&Cardona] Yu and Cardona, Fundamentals of Semiconductors(3rd), Springer (2003)
Sample
Source
Source
Analyzer
Analyzer
photon 0: absorption, reflection
photon photon : Raman scattering, Compton scattering, XES
photon electron : PES (XPS, UPS)
electron electron: electron energy loss spectroscopy
electron photon: inverse PES (BIS)
Electron excitations: examples
[Yu&Cardona]
Electron energy loss spectrum
Auger electron spectrum
Optical absorption
Photoelectron spectroscopy and optical absorption
[Jiang12]
Electronic band structure of semiconductors
[YuBook]
Mean field approaches
Remark: Kohn-Sham DFT is a many-body theory for the ground state total energy , but a mean-field approximation for single-electron excitation spectrum.
(Illustrations from G.-M. Rignanese’s talk)
The band gap problem
NiO
The origin of the DFT band gap problem
Perdew & Levy (1983); Sham & Schlueter (1983); Godby & Sham (1988)
KS HOMO-LUMO Gap ≠ Egap even with exact Exc
But for all explicit density functionals, e.g. LDA/GGA, Δxc=0
Quasi-particle theory
(courtesy of Dr. R. I. Gomez-Abal)
Concept of quasi-particles
[Mattuck]
quasi-particle theory and GW approximation
Quasi-particle equation
H. Jiang, Acta Phys.-Chim. Sin. 26, 1017(2010)
Green’s functions for single-electron Schrödinger Equations
Green’s function Green function
Definition of Green’s function (mathematically)
ˆ ( ) ( ) 0z H ψ − = r r
Consider a partial differential equation of the general form with a
certain boundary condition
z : a complex number
: a general Hermitian differential operator ˆ ( )H r
ˆ ( ) ( , '; ) ( ')z H G z δ − = − r r r r r
Green’s function G(r,r’;z) is defined as the solution of the following
equation with the same boundary condition for ψ(r):
Analytic properties of Green’s function ˆ ( ) ( , '; ) ( ')z H G z δ − = − r r r r r
*( ) ( ') ( ')n nnφ φ δ= − r r r rˆ ( ) ( ) ( )n n nH φ ε φ=r r r
* * *'( ) ( ') ( ) ( ') ( ) ( ')( , '; ) n n n n
n nn n
G z dz z z
ε εφ φ φ φ φ φ εε ε ε
= = +− − −
r r r r r rr r
G(r,r’;z) is analytic in the z-plane except at the eigenvalues of (discrete eigenvalues of ): simples poles (continuum eigenvalues of and extended states):
a branch cut
(continuum eigenvalues of and localized states): a natural boundary
( , '; ) ( , '; ), 0G G iε ε η η± ± += ± =r r r r
Green’s function for perturbation theory ˆ ( ) ( , '; ) ( ')z H G z δ − = − r r r r r
ˆ ( ) ( ) ( )
( , '; ) ( ') ', (z , )( )
( , '; ) ( ') ' ( ) (z= ) n
z H f
G z f dG f d ε
ψ
ε εψ
ε φ ε±
− = ≠
= +
r r r
r r r rr
r r r r r
0 0ˆ ( ) ( ; ) 0E H Eψ − = r r
0ˆ ( ) ( ) ( ; ) 0E H V Eψ − − = r r r 0
ˆ ( ) ( ; ) ( ) ( ; )E H E V Eψ ψ − = r r r r
0 ( , '; )G E± r r
0 0( ; ) ( ; ) ( , ') ( ') ( '; ) 'E E G V E dψ ψ ψ± ± ±= + r r r r r r r(Lippman-Schwinger equation)
Dyson’s equationIn many cases, we are interested in the perturbation expansion of
Green’s functions instead of that of wave functions
0 0
0
ˆˆ ( ) 1
ˆˆ ˆ ( ) 1
z H G z
z H V G z
− = − − =
1
0 00
1
00
1ˆ ˆ( ) ˆ
1ˆ ˆ ˆ( ) ˆ ˆ
G z z Hz H
G z z H Vz H V
−
−
= − ≡ −
= − − ≡ − −
10 0
10
ˆ ˆ( )ˆ ˆ ˆ( )
G z z H
G z z H V
−
−
= −
= − −1 1
0ˆ ˆ ˆ( ) ( )G z G z V− −= −
1 100 0
ˆ ˆ( ) (ˆ ˆ( )ˆ ˆ ˆ( ) ( )) ( )G z G z G z VGG zz G z− − = −
0 0ˆ ˆ ˆ(ˆ ˆ( ) ( )) ( )G G z G zz Vz G= + a Dyson’s equation
Time-dependent Green’s function
Time-dependent Schrödinger equation
ˆ ( ) ( , ) 0i H tt
ψ∂ − = ∂ r r
ˆ ( ) ( , ' ') ( ') ( ')i H G t t t tt
δ δ∂ − = − − ∂ r r r r r
For independent of time, , ≡ , ;Fourier transform ( ')1( , '; ') ( , '; )
2i t tG t t G e dωω ω
π+∞ − −
−∞− = r r r r
ˆ ( ) ( , '; ) ( ')H Gω ω δ − = − r r r r r
But: , ; is singular if ω is equal to any eigenvalue of !
(all in atomic units!)
Retarded and advanced Green’s function
ˆ ( ) ( , ' ') ( ') ( ')i H G t t t tt
δ δ∂ − = − − ∂ r r r r r
R/A / ( ')
( ')
1( , '; ') ( , '; )21 ( , '; )
2
i t t
i t t
G t t G e d
G i e d
ω
ω
ω ωπ
ω η ωπ
+ −+∞ − −
−∞
+∞ − −
−∞
− =
≡ ±
r r r r
r r
Retarded Green’s function
*( ) ( ')( , '; ) n n
n n
G zz
φ φε
=− r rr r
*R ( ) ( ')( , '; ) ( ) , ( ')nin n
n n
G i e t tz
ε τφ φτ θ τ τε
−= − ≡ −− r rr r
*A ( ) ( ')( , '; ) ( ) nin n
n n
G i ez
ε τφ φτ θ τε
−= −− r rr r
The use of Green’s function
R( , ) ( , '; ') ( ', ')t G t t t dΨ = − Ψr r r r r
Retarded Green’s function as the propagator
Density matrix
Eigenvalues from the poles of Green’s functions *( ) ( ')( , '; ) n n
n n
G zz
φ φε
=− r rr r
( )*
R/A
*
*( ) ( ') 1ˆ( , '; )
( ) ( ')
( ) ( ')
( , ';ˆ )
n n
n nn n
n n
n
n n n
n
G ii
i
φ φφ φω πω ε η ω ε
φ φ
δ ω ε
ρ ωπω ε
= = Ρ − ± −
−
= Ρ−
r rr r
r r
r r
r r
( )1 1ˆ i xx i x
πδη
= Ρ ±
R/A A R1 1( , '; ) Im ( , '; ) ( , '; ) ( , '; )2
G G Gρ ω ω ω ωπ π
= = − r r r r r r r r
Green’s function for many-body systems: General formalism
Outline
• Green’s functions: definition and properties
• Many-body perturbation theory based on Green’s functions
• Hedin’s equations
Representations (pictures) of quantum mechanics
Schrödinger Representation
( ) ( ) ( )
( ) ( ) ( )†
ˆ
( ) , ,
, ,
ˆS S
S
S
Si H qt
O t Oq
q t
q tqt dq
q tΨ∂ =∂
Ψ
Ψ
= Ψ
Heisenberg Representation
( )
( ) ( ) ( )( ) ( )
( ) ( )
H
†H H
H
H
H
ˆ ˆ
H
0
( )
ˆ ˆ, (assuming is independent of time)
ˆ ˆ ˆ, , ,
ˆ ,
ˆ , iHt iHtS
it
O t q q dq
e O q e H
i O q t O q t Ht
O q t
O q t
q
−
∂ =∂
= Ψ Ψ
=∂ = ∂
Ψ
Hamiltonian in terms of field operatorsField operators
Field operators in the Heisenberg representationˆ ˆ† †
ˆ ˆ
ˆ ˆ( ) ( )
ˆ ˆ( ) ( )
iHt iHt
iHt iHt
t e e
t e e
ψ ψ
ψ ψ
−
−
=
=
x x
x x
[ ] † †
†
ˆ ˆ ˆ ˆ( ), ( ') ( ), ( ') 0
ˆ ˆ( ), ( ') ( , ')
ψ ψ ψ ψ
ψ ψ δ+ +
+
= =
=
x x x x
x x x x
ˆ ( )ψ x†ˆ ( )ψ x
annihilation operator remove an electron at rcreation operator creator an electron at r
Hamiltonian of N-electron interacting systems
ˆ ˆ ˆˆ ˆ ˆ,
{ , }, : spin index
A B AB BA
s s+
≡ + ≡x r
20 ext
1ˆ ( ) ( )2
h V≡ − ∇ +x x
Definition of (one-body) Green’s function
†ˆ ˆ ˆ( , ' ') T ( ) ( ' ')G t t i N t t Nψ ψ = − x x x x
††
†
ˆ ˆ ( ) ( ' '), ' ˆ ˆ ˆT ( ) ( ' ')ˆ ˆ( ' ') ( ), '
t t t tt t
t t t tψ ψψ ψψ ψ
> = <±
x xx x
x x
N
T̂the ground state of the N-electron systemstime-ordering operator
† † †0
1ˆˆ ˆ ˆ ˆ ˆ ˆ ˆ( ) ( ) ( ) ' ( ') ( ) ( ' ) ( ' ) ( )2
H dx t h t d d v t t t tψ ψ ψ ψ ψ ψ= + − x x x x x r r x x x x
(one-body) Green’s function
Note:
Physical significance of Green’s function (1)
't t>†ˆ ( ', ')t Nψ x1) add an electron to the system at x’ and t’
†ˆ ˆ( , ) ( ', ')N t t Nψ ψx x3) project to the ground state (measure!)
†ˆ ˆ (( ', '), ) tt Nψ ψ xx2) take an electron away from the system
at x and t
Physical significance of Green’s function (2)† †ˆ ˆ ˆ ˆ( , ' ') ( ') ( ) ( ' ') ( ' ) ( ' ') ( )iG t t t t N t t N t t N t t Nθ ψ ψ θ ψ ψ= − − −x x x x x x
't t<1) remove an electron from (add a hole to )
the system at (x,t )
ˆ ( , )t Nψ x
2) add an electron to (annihilation of the
hole) the system at (x’,t’)
†ˆ ( ', ') ˆ ( , ) Nt tψψ xx
3) project to the ground state (measure!) †ˆ ˆ( ', ') ( , )t t NN ψ ψx x
Lehmann representation (1)
Lehmann representation (2)
metallic systems: Insulating systems:
Lehmann representation (3)
Lehmann representation (4)
fs(x): Lehmann (quasi-particle) amplitudes
Spectral representation of Green’s function
Spectral function
Spectral representation of Green’s function
Alternatively,
Quasi-particles
Spectral function
Non-interacting systems
Interacting systems
(Figures from G.-M. Rignanese’s talk)
Green’s function for many-body systems: General formalism
Outline
• Green’s functions: definition and properties
• Many-body perturbation theory and Hedin’s equations
Equation of motion for GFs
Equation of motion for GFs
Similar EOS can be derived for G2 which involves G3, and so on.
Two-body Green’s function
Equation of motion for GFs: Approximations
Hartree approximation
Hartree-Fock approximation
(exchange-correlation) self-energyDefinition:
Equation of Motion
Fourier transform
Dyson’s equation
Dyson’s equation (again!)
in matrix form
Hartree approximation
Quasi-particle Equation (?)
Quasi-particles
Two major approaches to obtain approximate Σxc
Diagrammatic expansion (Wick’s theorem)
Equation of motion and functional derivatives
0 H (( ) ( ) ( , ' ) ' ( , ' ) ( ' , ' ) )) (, = ' ( )i h V G t t d dt t t G t t t tttδ δ δδ
φ ′ ′ ′′ ′ ′′ ′ ′′ ′ ′− − + − Σ − − x x x x x x x x x x xx
Hedin’s Equations
(Figures from G.-M. Rignanese’s talk)
Hedin’s Equations: Derivation (1)
adiabatic small perturbation
Hedin’s Equations: Derivation (2)
Hedin’s Equations: Derivation (3)
Hedin’s Equations: Derivation (4)
Hedin’s Equations: Derivation (5)
Hedin’s Equations: Derivation (6)
Hedin’s Equations: Derivation (7)
Hedin’s Equations: the “grand pentagon”
Ground state properties from Green’s function (1)The expectation value of one-body operator
Examples:
In general, two-body physical properties cannot be obtained
directly from one-body Green’s function.
Exception:
Galitskii-Migdal formula
Ground state properties from Green’s function (2)
GW approximation and implementations
Outline
• GW approximation
• Implementations of the GW approach
H. Jiang, Front. Chem. China 6(4): 253–268 (2011)
GW Approximation
“best G best W” : G0W0 Approximation
Hybertsen and Louie(1985); Godby, Schlüter and Sham (1986)
( ) ( ) ( ) 'xc 0 0, '; , '; ' ', ; ' '
2ii G W e dηωω ω ω ω ω
πΣ = +r r r r r r
Implementation: main ingredients
*
*
0 0 0
,
,
*
( , '; ) = ( , '; ) ( ', ; )
1 1(1 ( ') ( ')
( ')
( ))
( )
( )
( )
2
= n mm n m nn
n mn m
nm m n
m
nmn
m
f f
P
i i
i d
F
G G
ψ
ω ω ω
ω ε ε η
ω ω
ω ε ε
ω
ψψη
π
ψ
− −
′ ′ ′
Φ
− + + + − − Φ
− +
≡
x x x x x
x
xx
x
x
x x
Polarization function
Key ingredients:
How to expand the products of two orbitals the product basis
How to treat frequency dependency
( ) 0xc
* *0 0
( )'
2 '
( ) ( ) ( ') ( , '; ) ( ) ( ') '
m k k nm n
k
i j k l i
k
j k l
Wi d
W W d d
ψ ψ ω ψ ψψ ω ψ ω
π ω ω
ψψ ω ψ ψ ψ ψ ω ψ ψ
εΣ =
+ −
=
r r r r r r r r
Self-energy
sgn( )k k kiε ε η μ ε= + −
Matrix representation
Product basis:
( ), , ,ε= ≡ −cO v P W W v
c
,
Zc
*B (1( ) '
, ) ( , ')2 '
( , )n
mc m
i jnm ij nm
i j
Md
WiN
Mωω ω
π ω ω ε+∞
−∞−
Σ
=−
+ k
q k q
k q q k q
( , ; ')nmX ωk q
GW implementations
Implementation: the product basis (1)
[ ]1( ) ( ) exp ( )χ χ→ ≡ + ⋅q qGr r q G ri i
VPlanewaves
;= ( )ψ χ kk k G G
Grn nc 1/2 *
; ' ; ''
( , ) =nm n mM V C C−− −G
k G k q G GG
k q
' , '1( ) = .
| |δ
+GG G Gqq G
v ' ' '4( , ) = ( , ).
| || ' |πε ω δ ω−
+ +GG GG GGq qq G q G
P
Codes: abinit, yambo, BerkeleyGW, SaX, vasp
Atomic-like orbitals ( )1/2
1( ) = ( )αα α αχ φ⋅ + − − q R tq
Rr r R ti
c
eN
[ ] *( ) ' ( ) ( , ' ( ')) .V Vd d Xα βαβ χ χ≡ qq r rr rX r r
[ ]1 1( ) = ( ) ( ) ( )− −qX Xq S q q S q
*( ) ( ) ( ).
VS dαβ α βχ χ ≡ q qq r r r
*
,
= ( ) ( ) (( , ) )' .X α βαβα βχ χ q q
qr r q rXr
Codes: FHI-aims, FIESTA
(L)APW+lo(+LO) basis
{ } { }MBmax, '
' ' ' '( ) ( ) ( )l ll l NLl l L l l
lu r u r v rαζ αζ≤
− ≤ ≤ +⎯⎯⎯⎯→
Mixed basis
MBmax
( )
( ),
ˆ( ) ( ), MT spheres
( ) 1 , Interstitial
iNL LM
G
i ii
e v r Y
S eV
α α α
αχ
⋅ +
+ ⋅
<
∈=
∈
q R r
Rq
q G rG
G
r r
rr
Implementation: the product basis (2)
Codes: GAP, SPEX
Implementation: frequency dependence
Static approximations
Coulomb hole-screened exchange (COHSEX)
Generalized plasmon pole (GPP) model
Full frequency treatment
Imaginary frequency + analytic continuation
real frequency Hilbert transform
Contour deformation
o*
'
o*
'
SE
*
0
c
X
R ( , '; ) =
( ) ( ') ( ', ( ', ; )1( ) ( ')
1 ( ' ) ( , ';0)2
; )
( ) ( ') ( ', ;0
(
)
' , )
cc
n n nn
cc
c
n
n
n
n nn
n
WdWe
WW
ψ ψ ω ωψ ψ ωπ ω
δψ ψ
εω
ωε
∞ ′ℑ′−′−
Σ
+
≡
− ℜ
+
−
−
− ℜ
Σ
−
k k kk
k kk
k kk k
r rr r
r
r r r r
r r r r
r
r r r
r
r
r
COH ( , ')Σ r r
frequency treatment: GPP modelsPlasmon pole model for homogeneous electron gas
1Im ( , ) ( ) ( ( ))pq A q qε ω δ ω ω− ≈ −
Generalized plasmon pole models
( )1' ' '
11 ' '
'2 2 2 20'
Im ( , ) = ( ) ( )
( ) ( )2 Im ( , ) 2Re ( , ) = = .( )
A
Ad
ε ω δ ω ωωω ε ωε ω ω δ
π ω ω π ω ω
−
−∞−
−
′′+ +′ − −
GG GG GG
GG GGGG
GG
q q q
q qqq 1q
Hybertsen-Louie (HL) model
Godby-Needs (GN) model
von der Linden-Horsch (vdLH) model
Engel-Farid model
frequency treatment : Hybertsen-Louie model
( )1' ' 'Im ( , ) = ( ) ( )Aε ω δ ω ω− −GG GG GGq q q
Two parameters for each G, G’ are determined by
1) Static dielectric function ω=0
2) The f-sum rule 1 2
' '0
2'
Im ( , ) = ( )2
4 ( ) ( ')( ) ( ')| || ' |
d πω ε ω ω
π ρ
∞ − − Ω
+ ⋅ +Ω = −+ +
GG GG
GG
q q
q G q Gq G Gq G q G
1/21' ' ' '
'' 1/21
' '
( ) = ( ,0) | |2
| |( ) =( ,0)
π δ ε
ωδ ε
−
−
− Ω
Ω −
GG GG GG GG
GGGG
GG GG
q q
A
frequency treatment : the GN model
( )1' ' 'Im ( , ) = ( ) ( )Aε ω δ ω ω− −GG GG GGq q q
Two parameters for each G, G’ are determined by
1) Static dielectric function ω=0
2) Inverse dielectric at a chosen imaginary frequency, ω=iωp
( )( )1/2 1 1 1 1/2' ' ' ' '
1/21 1' '1/2
' 1' '
( ) = [ ( ,0) ( ,0) ( , ) ]2
( ,0) ( , )( ) =
( ,0)
p p
pp
A i
i
π ω δ ε ε ε ω
ε ε ωω ω
δ ε
− − −
− −
−
− −
− −
GG GG GG GG GG
GG GGGG
GG GG
q q q q
q qq
q
frequency dependence: IF+AC approach
Imaginary frequency plus analytic continuation (IF-AC) o u *
2 2
2( )( , ) = 2 ( , ) ( , )
( )
BZ cc noccn n i j
ij nm nmn m n n
P iu M Mu
ε εε ε
−
−
− − × + − k k q
k k k q
q k q k q
( )( )
c20 2
2 ( , ; )( ) = .
2ε
π ε
∞ −
−
′−′Σ
′ + − k q
kq k q
k qBZm nm
nm m
iu X iuduiuu iu
p;c
;
( ) =N
p nn
p p n
aiu
iu bΣ
− kk
k
p;c
;
( ) =N
p nn
p p n
ab
ωω
Σ− k
kk
frequency dependence : the CD approach
Contour deformation (CD) approach c
F
( )( ) = .2 sgn( )
nmn
m m m
Xi diωω ω
π ω ω ε η ε ε∞
−∞
′′Σ′+ − − −
c2 20
F F
2( )( ) ( )2 ( )
( )[ ( ) ( ) ( ) ( )]
mn nm
m m
nm m m m m m
du X iuu
X
ε ωωπ ε ω
ε ω θ ε ε θ ω ε θ ε ε θ ε ω
∞ −Σ =− +
+ − − − − − −
Self-consistency: full vs approximate SCGW
Full SCGW Approx. SCGW
Faleev-van Schilfgaarde-Kotani (QSGW) scheme (PRL 2004)
Main technical parameters in GW implementation
Parameters for KS DFT:
pseudopotentials, PAW or LAPW?
basis for Kohn-Sham orbitals
Quality of product basis
Number of unoccupied states considered (P & Σc )
The integration in the Brillouin zone: the number of k/q-
points
The frequency treatment and related parameters
H. Jiang, Front. Chem. China 6(4): 253–268 (2011)
Examples for applications of the GW approach
Band gaps of semiconductors
H. Jiang: GW with HLOs-enhanced LAPW (unpublished)
M. van Schilfgaarde et al. PRL
96, 226402 (2006)
72
GW0@LDA for ZrO2 and HfO2
Jiang, H. et al. Phys. Rev. B 81, 085119 (2010)
Band gaps of MX2 and ATaO3
Jiang, H., J. Chem. Phys , 134, 204705 (2011);Jiang, H. J. Phys. Chem. C,116, 7664 (2012).
Pm-3m R3ch
H. Wang, F. Wu and H. Jiang, J. Phys. Chem. C, 115, 16180, (2011)
Ln2O3 band gaps: GW0@LDA+U vs Expt.
H. Jiang et al. Phys. Rev. Lett. 102, 126403(2009); Phys. Rev. B 86, 125115(2012).
Fully self-consistent GW for molecules
Rostgaard, Jacobsen and Thygesen, PRB 81, 085103 (2010)
GW for fullerenes
GW for CuPc
Level alignment in dye-sensitized solar cells
P. Umari et al. J. Chem. Phys. 139, 014709 (2013)C. Verdi et al, Phys. Rev. B 90, 155410 (2014)