I.Overview

1.Statistical Physics for Equilibrium

Microcanonical Ensemble

P=1/WP=1 / W

Isolated systems with constant N, V, E

Canonical Ensemble

P(E)=e(FE)/KTP(E)=e^{(F-E) / K T}

Systems in contact with a heat bath (constant N,V,T\mathrm{N}, \mathrm{V}, \mathrm{T} )

Grand Canonical Ensemble

P(E,N)=e(Ω+μNE)/KTP(E, N)=e^{(\Omega+\mu N-E) / K T}

Systems that have exchange of particles and energies with environment (constant V,T\mathrm{V}, \mathrm{T} and μ\mu )

2.Nonequilibrium and Equibrium

Equilibrium

Average values of physical properties do not vary with time and independent from momentum of particles.

Nonequilibrium processes

  • Time-dependent processes
    Phase changes; Chemical reactions; Any system changes due to external forces.
  • Steady-state Transport processes
    Mass transport; Charge transport; Spin transport; Heat transport.

3.Equilibrium state and Steady state

Equilibrium State

  • Associated with a particular temperature T
  • The system has a universal chemical potential
  • Average values of physical measurables do not vary with time

Steady State

  • Average values of physical measurables do not vary with time
  • Can be in equilibrium or nonequilibrium

4.Typical nonequilibrium phenomena in electronic materials

Materials: Ions + Electrons

Time-dependent (TD) processes

  • TD Ion motions: Structure phase changes; Chemicalreactions.
  • TD Electron properties: Electronic phase changes; Electronic excitations.

Steady-state Transport processes

  • DC electric/spin current: Transport of electrons or ions.
  • Thermoelectric effects: Electron and heat transport.

II.Equilibrium Modelling: Density Functional Theory and Kohn-Sham Approach

1.Emerging of DFT

The central issue for understanding materials

H^ψ=EψAˉ=ψA^ψ\hat{H} \psi=E \psi \quad \Longrightarrow \bar{A}=\langle\psi| \hat{A}|\psi\rangle

H^=h22mii21κm;i=1,Neqmrim+1κi;j>ie2rij\hat{H}=-\frac{\mathrm{h}^2}{2 m} \sum_i \nabla_i^2-\frac{1}{\kappa} \sum_{m ; i=1, N} \frac{e q_m}{r_{i m}}+\frac{1}{\kappa} \sum_{i ; j>i} \frac{e^2}{r_{i j}}

1st Hohenberg-Kohn (HK) theorem (1965)
The Hamiltonian of a quantum system is determined, within a trivial constant, by the ground-state electron density ρ(r)\rho(r).

Aˉ=A[ρ(r)]\Longrightarrow \bar{A}=A[\rho(r)]

2nd Hohenberg-Kohn (HK) theorem
For an arbitrary electron density ρ~(r)\widetilde{\rho}(r) such that ρ~(r)0,ρ~(r)dr=N\widetilde{\rho}(r) \geq 0, \int \widetilde{\rho}(r) d r=N, the ground-state energy E0E_0 is always lesser than E~[ρ~]\widetilde{E}[\widetilde{\rho}] when this arbitrary density is different from the ground-state density.

DFT Variational Principle

E[ρ]=T^[ρ]+V^ext[ρ]+V^ee[ρ]=V^ext[ρ]+FHK[ρ]E[ρ]Min{ρV^exp[ρ]+FHK[ρ]}\begin{gathered} E[\rho]=\hat{T}[\rho]+\hat{V}_{e x t}[\rho]+\hat{V}_{e e}[\rho]=\hat{V}_{e x t}[\rho]+F_{H K}[\rho] \\ E[\rho] \rightarrow \operatorname{Min} \{ _\rho \hat{V}_{\exp }[\rho]+F_{H K}[\rho] \} \end{gathered}

Assumption: A non-interacting reference system

ψ~GS=1N!det(φ1φ2φ3φN)ρ~reference =ψ~GS(r)2ρtrue GS\widetilde{\psi}_{G S}=\frac{1}{\sqrt{N!}} \operatorname{det}\left(\varphi_1 \varphi_2 \varphi_3 \ldots \varphi_N\right) \quad \quad \widetilde{\rho}_{\text {reference }}=\left|\widetilde{\psi}_{G S}(r)\right|^2 \equiv \rho_{\text {true } G S}

Approximate the kinetic energy of the true system by the kinetic energy of the reference system.

T[ρ]T~[ρ]iφi12i2φiT[\rho] \approx \widetilde{T}[\rho] \equiv \sum_i\left\langle\varphi_i\right|-\frac{1}{2} \nabla_i^2\left|\varphi_i\right\rangle

Search the non-interacting reference system
Variational Principle

E[ρ]=iφi12i2φi+ρ(r)Vext(r)dr+J[ρ]+Exc[ρ]φiφjdr=δijρ(r)=iφi(r)2Ω({φi})E[ρ]i,jεijφiφjdr\begin{aligned} & E[\rho]=\sum_i\left\langle\varphi_i\right|-\frac{1}{2} \nabla_i^2\left|\varphi_i\right\rangle+\int \rho(r) V_{e x t}(r) d r+J[\rho]+E_{x c}[\rho] \\ & \int \varphi_i \varphi_j d r=\delta_{i j} \quad \rho(r)=\sum_i\left|\varphi_i(r)\right|^2 \\ & \Omega\left(\left\{\varphi_i\right\}\right) \equiv E[\rho]-\sum_{i, j} \varepsilon_{i j} \int \varphi_i \varphi_j d r \end{aligned}

δΩ({φi})δ{φi}=0\frac{\delta \Omega\left(\left\{\varphi_i\right\}\right)}{\delta\left\{\varphi_i\right\}}=0

Kohn-Sham equation

(122+Veff )φi=εiφi\left(-\frac{1}{2} \nabla^2+V_{\text {eff }}\right) \varphi_i=\varepsilon_i \varphi_i

Veff(r)=Vext(r)+ρ(r)rrdr+Vxc(r)V_{e f f}(r)=V_{e x t}(r)+\int \frac{\rho\left(r^{\prime}\right)}{\left|r-r^{\prime}\right|} d r^{\prime}+V_{x c}(r)

Vxc(r)=δExc[ρ]δρV_{x c}(r)=\frac{\delta E_{x c}[\rho]}{\delta \rho}

2.Self-consistent Procedure

  • Given initial density

  • Build effective K-S potential

  • Solve K-S equation

  • Calculate density

III.Periodic Systems and Pseudopotential

Understanding periodic systems is the basis of modelling materials in equilibrium.

1.Bloch theorem in 1D

For a periodic system, H^(x+na)=H^(x)\widehat{H}(x+n a)=\widehat{H}(x),
Introduce a translational operator, T^(na)φ(x)=φ(x+na)\hat{T}(n a) \varphi(x)=\varphi(x+n a).
We can prove that T^\widehat{T} and H^\widehat{H} commute, [T^,H^]=0[\widehat{T}, \widehat{H}]=0.
Then, T^\widehat{T} and H^\widehat{H} shall have simultaneous eigen states,

H^ψ(x)=Eψ(x)T^(na)ψ(x)=Tψ(x)T^(na)ψ(x)=ψ(x+na)Tψ(x)=ψ(x+na)Tψ(x)2=ψ(x+na)2T=eiα(na)\begin{gathered} \widehat{H} \psi(x)=E \psi(x) \\ \widehat{T}(n a) \psi(x)=T \psi(x) \quad \widehat{T}(n a) \psi(x)=\psi(x+n a) \\ \mathrm{T} \psi(x)=\psi(x+n a) \\ |\mathrm{T} \psi(x)|^2=|\psi(x+n a)|^2 \Longrightarrow T=e^{i \alpha(n a)} \end{gathered}

Bloch Theorem:

ψ(x)=eikxϕ(x)\quad \boldsymbol{\psi}(\boldsymbol{x})=\boldsymbol{e}^{\boldsymbol{i} \boldsymbol{k} \boldsymbol{x}} \boldsymbol{\phi}(\boldsymbol{x})

ϕ(x+na)=ϕ(x)\phi(x+n a)=\phi(x)