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Nonlinear response  of solids
with Green's functions and TD­D(P)FT
Claudio Attaccalite 
CINaM, Aix­Marseille Universite (FR) 
 Myrta Grüning, Queen's University, Belfast(UK)
Theory Days - Toulouse - 26-11-2015Theory Days - Toulouse - 26-11-2015
What is it non­linear optics?
P(r ,t)=P0+χ
(1)
E+χ
(2)
E
2
+O(E
3
)
First experiments on linear­optics 
by P. Franken 1961
Ref: Nonlinear Optics and 
Spectroscopy 
The Nobel Prize in Physics 1981
Nicolaas Bloembergen
Ref: supermaket
Why non­linear optics?
..applications..
Ref: supermaket
Why non­linear optics?
..applications..
“Self­focusing limit in terms of peak power is of the order 
of 4 MW in the 1­μm wavelength region. No method is known 
for increasing the self­focusing limit of optical fibers 
beyond that value.”  RP Photonics
Why non­linear optics?
..applications.. (the darkside      )
Why non­linear optics?
..research..
Linear
Science, 2014, vol. 344, no 6183, p. 488­490
Non­linear(COLOR)Non­linear(BW)
To see “invisible” excitations
The Optical Resonances in 
Carbon 
Nanotubes Arise
from Excitons
Feng Wang, et al.
Science 308, 838 (2005);
..research..
...and more...
photon entanglement  in vivo imaging
Ref: PNAS 107, 14535 (2007) 
How to calculate non­linear 
response?
1) Direct evaluation of X(1)
,X(2)
....
2) Sternheimer equation
 R. M. Sternheimer, Phys. Rev. 96, 951(1954)
3) Real­time propagation
P(t)=P0+χ
(1)
E+χ
(2)
E
2
+O(E
3
)
(HKS
0
−ϵn
0
)ψn
1
=(H KS
1
−ϵn
1
)ψn
0
χ=χ
0
+χ
0
(v+f xc)χ
−i∂t ψ=Hks ψ
1) Equations become more and more complex 
with the response order
2) Difficult to include more than one  
external field (FWM, etc..)
Ref: PRB 80, 165318(2009),  PRA 83, 062122(2001),
     JCP 126, 184106(2007)
 Direct evaluation of X(1)
,X(2)
....
Disadvantages:
 Sternheimer equation
Advantages
Ref: JCP, 127, 154114(2007)
     PRB, 89,  081102(2014)
 Real­time propagation
1) The same equation for all response 
functions
2) Can deal with complex spectroscopic 
tecniques (SFG, FWM, etc...)
Disadvantages
1) Results are more difficult to analize 
What to propagate?
(Current) Density Density Matrix
 Green's function Wave function
The best chioce for solids is.....
Wave function
Why?
1)We know  how to express polarization in terms of 
the wave­function (the King­Smith Vanderbilt formula).
R. D. King­Smith and D. Vanderbilt, PRB 47, 1651 (1993)
2)Polarization in terms of Green's function or 
density matrix is very complicated
 K.­T. Chen and P. A. Lee, PRB 84, 205137 (2011)
3)Polarization in terms of the density is impossible!
   R. M. Martin and G. Ortiz, PRB 56, 1124(1997)
From Polarization to the 
Equations of Motion
I. Souza, J. Iniguez and D. Vanderbilt, PRB 69, 085106 (2004)
Pα=
2ie
(2π)
3 ∫BZ
d k∑n=1
nb
〈un k∣
∂
∂ kα
∣unk 〉
King­Smith and Vanderbilt formula
Phys. Rev. B 47, 1651 (1993)
L=
i ℏ
N
∑n=1
M
∑k
〈 vkn∣˙vkn〉−〈H
0
〉−v Ε⋅P
Once we know how to write the polarization we 
can define a Lagrangian
i ℏ ∂
∂t
|vk n⟩=Hk
0
|vk n⟩+i e Ε⋅|∂k vk n⟩
From the Lagrangian we derive the Hamiltonian
and the Eqs. of motion
Correlation
Ref: PRB 84, 245110(2011),PRB 25, 2867 (1982)
     L. P. Kadanoff & G. A. Baym, 
     Quantum statistical mechanics, Benjamin(1962).
     G. Strinati, La Rivista del Nuovo Cimento, 11,1­86 (1998)
Correlation effects are derived 
from non­equilibrium Green's 
theory within the GW approximation 
GW band structure
Aryasetiawan, F., & Gunnarsson, O. The GW method.
Reports on Progress in Physics, 61(3), 237.(1998).
W (ω)=
V ee
ϵ(ω)
GW is the first
order correction in
terms of screened
interaction
H=H0+Δi, jk
GW
Δi, jk
GW
=⟨ΣGW ⟩i, jk
Mapping GW in an effective Hamiltonian
Bethe­Salpeter Equation
+ -=
G. Strinati, Rivista del Nuovo Cimento, 11, 1 (1988)
C. Attaccalite, M Gruning and A. Marini PRB, 84, 245110 (2011)
L=L0+L0[v+ δ Σ
δG
] L Exact Bethe-Salpeter (useless)
L=L0+ L0[v−W ]LApprox. Bethe-Salpeter (usefull)
H=H0+Σ
COHSEX
[ ^ρ(t=0)−^ρ(t)]
Mapping BSE in an effective Hamiltonian
∂ Σ
COHSEX
∂V ext
Our computational setup
Correlation:
Green's function 
theory (GW+BSE)
Coupling:
Modern­Theory of 
Polarization
Ref: PRB 88, 235113(2013)
Linear response
Technical details:
● Wave­function in plane­waves plus norm­conserving pseudo
● Propagation time about 50 fs, with a time­step 0.01 fs
● Smearing included as non­Hermitian operator ­iγ (Weisskopf­Wigner)
or in post­processing as in Octopus
● Laser shape: delta function for LR/ sinus for Non­LR 
X(2)
results: semiconductors 
CdTe
Ref: 
E. Luppi el al.,PRB 82, 235201 (2010)
E. Ghahramani et al., PRB 43, 9700 (1991) 
I. Shoji,et al. J.Opt.Soc.Am. B 14, 2268 (1997) 
J.I.Jang,et al. J.Opt.Soc. Am.B 30, 2292 (2013)
M. Grüning at al. PRB 88, 235113(2013)
AlAs
Local field effects are 
more important than in 
the linear reposonse
Local­fields and excitonic effects
in h­BN monolayer
IPA
IPA + GW + TDSHF
independent particles
+quasi-particle corrections
+time-dependent Hartree (RPA)
+screend Hartree-Fock (excitonic effects)
MoS2 
single­layer
10) Second harmonic microscopy of monolayer MoS2
Phys. Rev. B 87, 161403(R) (2013)
100) Probing Symmetry Properties of Few­Layer MoS2
 and h­
BN by Optical Second­Harmonic Generation
NanoLetters, 13, 3329 (2013)
1000) Observation of intense second harmonic generation 
from MoS2
 atomic crystals
Phys. Rev. B 87, 201401(R) (2013)
X(3)
in silicon
Ref: PRB 41, 1542 (1990) 
     Optical letters, 14,57 (1989)
     PRB 88, 235113(2013) 
 X(3) 
in nanostructures
Interference between excitons 
is not trivial the case of ANGR7
Ref: Nature Comm. 5, 4253 (2014)
     PRL 94, 047404 (2005) 
TD­D(P)FT … why and why not?
TDDFT is much faster than Green's functions
Runge­Gross theorem does not hold in periodic 
system  (PRB 68, 045109)
Density is not enough to describe the response of 
periodic systems (PRB 56, 1124)
q⋅P(q)=in(q)
Current­density­FT works :­)
If there are not magnetic fields and 
transverse reponse is not important it 
reduces to
Density­Polarization­FT Exc(P ,n)
Searching for a functional
● We want a functional of the density and Polarization
● No functionals of the density only
● We do not want the exchange
● No divergences 1/q^2 etc...
Checklist:
Electron gas with gap (JGM)
P. Trevisanutto et al. 
PRB 87, 205143(2013)
Dielectric constant
Corresponding exchange­corr functional
(with a Micro and Macroscopic contribution)
We map the Macroscopic part in a 
functional of the polarization and the 
microscopic part in a functional of the 
density
N. T. Maitra, I. Souza, and K. Burke PRB 68, 045109
 Some preliminary results 
of the JGM functional
What we miss? 
Exc (t )=f xc (n)+α P (t )+β P
2
(t )+ γ P
3
(t)+....
For linear optics For χ2, χ3... For χ3,χ4,....
It can be shown that second term is as large as 
local field effects(PRB 54, 8540)  
First problem
Second problem
α(t)
In principle all the coefficients depend on time.
This is important to describe complex excitons, etc... 
 
β(t) γ(t)
Prospectives
Applications:
Developement:
● An exchange­correlation function beyond  linear 
response (that works)
● Spin and spin­orbit coupling
● Therahertz spectroscopy
● THG and Kerr parameters
● SHG and spin
● Electro­absorption
● Interfaces 
Conclusions
Develop an approach that 
'imports' successful GW+BSE 
recipe into versatile real­time 
approach:
correlation in nonlinear­optics
e­laser interaction treated 
within modern polarization theory
e­h interaction key to 
understand 
SHG spectra of 2D materials 
(such as hBN, MoS2)
Density­polarization 
functional theory
for the linear­response
JGM and beyond
Acknowledgement:
Myrta Grüning, 
Queen's University Belfast
Related work:
Implementation of dynamical Berry phase: 
C. Attaccalite, M. Grüning, PRB 88, 235113 (2013) 
Application to SHG of 2D materials: 
M. Grüning. C. Attaccalite, PRB 89(R), 081102 (2014)
C. Attaccalite et al., PCPC 17, 9533 (2015)
Time­dependent BSE theory: 
C. Attaccalite ,M. Grüning. A. Marini PRB 84, 245110 (2011)
Time­dependent density polarization theory: 
M. Grüning, D. Sangalli and C. Attaccalite, in preparation(2015)
The codes: 
A. Marini et al. Comp. Phys. Comm. 180, 1392 (2009)
P. Giannozzi et al. J. of Phys.: Cond. Matter, 21, 395502 (2009)
Does the velocity gauge make 
the life easier?
It is true if you have a local Hamiltonian 
Length gauge:
H =
p2
2 m
+r E+V (r)
Ψ(r ,t )
Velocity gauge:
H =
1
2 m
( p−e A)2
+V (r)
e
−i r⋅A(t)
Ψ(r ,t)
Analitic demostration:
K. Rzazewski and R. W. Boyd, 
J. of Mod. optics 51, 1137 (2004)
W. E. Lamb, et al. 
Phys. Rev. A 36, 2763 (1987)
Well done velocity gauge:
M. Springborg, and B. Kirtman
Phys. Rev. B 77, 045102 (2008) 
V. N. Genkin and P. M. Mednis
Sov. Phys. JETP 27, 609 (1968)
... but when you have non­local pseudo, exchange,
damping term etc..  
they do not commute with the  phase factor
The King­Smith Vanderbilt 
polarization 
King­Smith and Vanderbilt formula
Phys. Rev. B 47, 1651 (1993)
Pα=
2ie
(2π)
3 ∫BZ
d k∑n=1
nb
〈un k∣
∂
∂ kα
∣unk 〉
Berry's connection !!
1) it is a bulk quantity
2) time derivative gives the current
3) reproduces the polarizabilities at all orders
4) is not an Hermitian operator
Post­processing real­time data
P(t) is a periodic function of period TL
=2p/wL
 
pn
  is proportional to χn
by the n­th order of the external field 
Performing a discrete­time signal
sampling we reduce the problem to 
the solution of a systems of linear equations
Ref: PRB 88, 235113(2013), 
    JCP 138, 064104(2013) 

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Nonlinear response of solids with Green's functions and TD-D(P)FT

Notes de l'éditeur

  1. The light in a fiber-optic cable travels through the core (hallway) by constantly bouncing from the cladding (mirror-lined walls), a principle called total internal reflection. Because the cladding does not absorb any light from the core, the light wave can travel great distances.
  2. the Sternheimer equation requires only knowledge of the occupied states in order to determine the first order correction to the Kohn-Sham orbitals
  3. In fact, the IPA+GW shows two peaks: the first at about 4 eV is the shifted two-photon π → π∗ resonances peak which is attenuated by 40% with respect to IPA [Fig. 2 (a)]; the second very pronounced peak at about 8 eV comes from the interference of π → π ∗ one-photon resonances and σ → σ∗ two-photon resonances.
  4. MoS2 differs from h-BN in several aspects. First, while the h-BN has an indirect minimum band gap as its bulk counterpart, in MoS2 an indirect-to-direct bandgap transition occurs passing from the bulk to the monolayer due to the vanishing interlayer interaction. Second, spin-orbit coupling plays an important role in this material, splitting the top valence bands, as visible from the absorption spectrum, presenting a double peak at the onset.7 Third, Mo and S atoms in the MoS2 monolayer are on different planes resulting in a larger inhomogeneity than for the H-BN. gap at the K point; a larger peak around 1.5 eV, which originates from two-photon resonances with transitions along the high symmetry axis between Γ and K where the highest valence and lowest conduction bands are flat and there is a high density of states; a broad structure between 2−3.5 eV which originates from one-photon res-