I.Overview
1.Statistical Physics for Equilibrium
Microcanonical Ensemble
P = 1 / W P=1 / W
P = 1 / W
Isolated systems with constant N, V, E
Canonical Ensemble
P ( E ) = e ( F − E ) / K T P(E)=e^{(F-E) / K T}
P ( E ) = e ( F − E ) / K T
Systems in contact with a heat bath (constant N , V , T \mathrm{N}, \mathrm{V}, \mathrm{T} N , V , T )
Grand Canonical Ensemble
P ( E , N ) = e ( Ω + μ N − E ) / K T P(E, N)=e^{(\Omega+\mu N-E) / K T}
P ( E , N ) = e ( Ω + μ N − E ) / K T
Systems that have exchange of particles and energies with environment (constant V , T \mathrm{V}, \mathrm{T} V , T and μ \mu μ )
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 = E ψ ⟹ A ˉ = ⟨ ψ ∣ A ^ ∣ ψ ⟩ \hat{H} \psi=E \psi \quad \Longrightarrow \bar{A}=\langle\psi| \hat{A}|\psi\rangle
H ^ ψ = E ψ ⟹ A ˉ = ⟨ ψ ∣ A ^ ∣ ψ ⟩
H ^ = − h 2 2 m ∑ i ∇ i 2 − 1 κ ∑ m ; i = 1 , N e q m r i m + 1 κ ∑ i ; j > i e 2 r i j \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}}
H ^ = − 2 m h 2 i ∑ ∇ i 2 − κ 1 m ; i = 1 , N ∑ r i m e q m + κ 1 i ; j > i ∑ r i j e 2
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) ρ ( r ) .
⟹ A ˉ = A [ ρ ( r ) ] \Longrightarrow \bar{A}=A[\rho(r)]
⟹ A ˉ = A [ ρ ( r ) ]
2nd Hohenberg-Kohn (HK) theorem
For an arbitrary electron density ρ ~ ( r ) \widetilde{\rho}(r) ρ ( r ) such that ρ ~ ( r ) ≥ 0 , ∫ ρ ~ ( r ) d r = N \widetilde{\rho}(r) \geq 0, \int \widetilde{\rho}(r) d r=N ρ ( r ) ≥ 0 , ∫ ρ ( r ) d r = N , the ground-state energy E 0 E_0 E 0 is always lesser than E ~ [ ρ ~ ] \widetilde{E}[\widetilde{\rho}] E [ ρ ] when this arbitrary density is different from the ground-state density.
DFT Variational Principle
E [ ρ ] = T ^ [ ρ ] + V ^ e x t [ ρ ] + V ^ e e [ ρ ] = V ^ e x t [ ρ ] + F H K [ ρ ] E [ ρ ] → Min { ρ V ^ exp [ ρ ] + F H K [ 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}
E [ ρ ] = T ^ [ ρ ] + V ^ e x t [ ρ ] + V ^ e e [ ρ ] = V ^ e x t [ ρ ] + F H K [ ρ ] E [ ρ ] → M i n { ρ V ^ e x p [ ρ ] + F H K [ ρ ] }
Assumption: A non-interacting reference system
ψ ~ G S = 1 N ! det ( φ 1 φ 2 φ 3 … φ N ) ρ ~ reference = ∣ ψ ~ G S ( r ) ∣ 2 ≡ ρ true G S \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}
ψ G S = N ! 1 d e t ( φ 1 φ 2 φ 3 … φ N ) ρ reference = ∣ ∣ ∣ ∣ ψ G S ( r ) ∣ ∣ ∣ ∣ 2 ≡ ρ true G S
Approximate the kinetic energy of the true system by the kinetic energy of the reference system.
T [ ρ ] ≈ T ~ [ ρ ] ≡ ∑ i ⟨ φ i ∣ − 1 2 ∇ i 2 ∣ φ i ⟩ T[\rho] \approx \widetilde{T}[\rho] \equiv \sum_i\left\langle\varphi_i\right|-\frac{1}{2} \nabla_i^2\left|\varphi_i\right\rangle
T [ ρ ] ≈ T [ ρ ] ≡ i ∑ ⟨ φ i ∣ − 2 1 ∇ i 2 ∣ φ i ⟩
Search the non-interacting reference system
Variational Principle
E [ ρ ] = ∑ i ⟨ φ i ∣ − 1 2 ∇ i 2 ∣ φ i ⟩ + ∫ ρ ( r ) V e x t ( r ) d r + J [ ρ ] + E x c [ ρ ] ∫ φ i φ j d r = δ i j ρ ( r ) = ∑ i ∣ φ i ( r ) ∣ 2 Ω ( { φ i } ) ≡ E [ ρ ] − ∑ i , j ε i j ∫ φ i φ j d r \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}
E [ ρ ] = i ∑ ⟨ φ i ∣ − 2 1 ∇ i 2 ∣ φ i ⟩ + ∫ ρ ( r ) V e x t ( r ) d r + J [ ρ ] + E x c [ ρ ] ∫ φ i φ j d r = δ i j ρ ( r ) = i ∑ ∣ φ i ( r ) ∣ 2 Ω ( { φ i } ) ≡ E [ ρ ] − i , j ∑ ε i j ∫ φ i φ j d r
δ Ω ( { φ i } ) δ { φ i } = 0 \frac{\delta \Omega\left(\left\{\varphi_i\right\}\right)}{\delta\left\{\varphi_i\right\}}=0
δ { φ i } δ Ω ( { φ i } ) = 0
Kohn-Sham equation
( − 1 2 ∇ 2 + V eff ) φ i = ε i φ i \left(-\frac{1}{2} \nabla^2+V_{\text {eff }}\right) \varphi_i=\varepsilon_i \varphi_i
( − 2 1 ∇ 2 + V eff ) φ i = ε i φ i
V e f f ( r ) = V e x t ( r ) + ∫ ρ ( r ′ ) ∣ r − r ′ ∣ d r ′ + V x c ( 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)
V e f f ( r ) = V e x t ( r ) + ∫ ∣ r − r ′ ∣ ρ ( r ′ ) d r ′ + V x c ( r )
V x c ( r ) = δ E x c [ ρ ] δ ρ V_{x c}(r)=\frac{\delta E_{x c}[\rho]}{\delta \rho} V x c ( r ) = δ ρ δ E x c [ ρ ]
2.Self-consistent Procedure
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 + n a ) = H ^ ( x ) \widehat{H}(x+n a)=\widehat{H}(x) H ( x + n a ) = H ( x ) ,
Introduce a translational operator, T ^ ( n a ) φ ( x ) = φ ( x + n a ) \hat{T}(n a) \varphi(x)=\varphi(x+n a) T ^ ( n a ) φ ( x ) = φ ( x + n a ) .
We can prove that T ^ \widehat{T} T and H ^ \widehat{H} H commute, [ T ^ , H ^ ] = 0 [\widehat{T}, \widehat{H}]=0 [ T , H ] = 0 .
Then, T ^ \widehat{T} T and H ^ \widehat{H} H shall have simultaneous eigen states,
H ^ ψ ( x ) = E ψ ( x ) T ^ ( n a ) ψ ( x ) = T ψ ( x ) T ^ ( n a ) ψ ( x ) = ψ ( x + n a ) T ψ ( x ) = ψ ( x + n a ) ∣ T ψ ( x ) ∣ 2 = ∣ ψ ( x + n a ) ∣ 2 ⟹ T = e i α ( n a ) \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}
H ψ ( x ) = E ψ ( x ) T ( n a ) ψ ( x ) = T ψ ( x ) T ( n a ) ψ ( x ) = ψ ( x + n a ) T ψ ( x ) = ψ ( x + n a ) ∣ T ψ ( x ) ∣ 2 = ∣ ψ ( x + n a ) ∣ 2 ⟹ T = e i α ( n a )
Bloch Theorem :
ψ ( x ) = e i k x ϕ ( x ) \quad \boldsymbol{\psi}(\boldsymbol{x})=\boldsymbol{e}^{\boldsymbol{i} \boldsymbol{k} \boldsymbol{x}} \boldsymbol{\phi}(\boldsymbol{x})
ψ ( x ) = e i k x ϕ ( x )
ϕ ( x + n a ) = ϕ ( x ) \phi(x+n a)=\phi(x)
ϕ ( x + n a ) = ϕ ( x )