14. 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
16. 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
17. 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
29. 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)
33. 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 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.
the Sternheimer equation requires only knowledge of the occupied states in order to determine the first order correction to the Kohn-Sham orbitals
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.
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-