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Electronic Band Structure

5.1 Free Electron Model

In the simplest model, conduction electrons move freely in a box of volume VV (the “jellium” model). The allowed wave vectors are:

k=2πL(nx,ny,nz),niZ\mathbf{k} = \frac{2\pi}{L}(n_x, n_y, n_z), \quad n_i \in \mathbb{Z}

The energy spectrum:

ε(k)=2k22me\varepsilon(\mathbf{k}) = \frac{\hbar^2 k^2}{2m_e}

The Fermi wave vector is determined by the electron density n=N/Vn = N/V:

kF=(3π2n)1/3k_F = (3\pi^2 n)^{1/3}

The Fermi energy:

εF=2kF22me\varepsilon_F = \frac{\hbar^2 k_F^2}{2m_e}

5.2 Density of States

For a 3D free electron gas:

g(ε)=V2π2(2me2)3/2εg(\varepsilon) = \frac{V}{2\pi^2}\left(\frac{2m_e}{\hbar^2}\right)^{3/2}\sqrt{\varepsilon}

Derivation. The number of states with kk\lvert\mathbf{k}\rvert \leq k is:

N(k)=2V(2π)34πk33N(k) = 2 \cdot \frac{V}{(2\pi)^3} \cdot \frac{4\pi k^3}{3}

Where the factor of 2 accounts for spin. Differentiating: g(k)dk=dN/dkdk=(Vk2/π2)dkg(k)\,dk = dN/dk\,dk = (Vk^2/\pi^2)\,dk. Converting to energy: g(ε)=g(k)dk/dε=(Vk2/π2)(me/2k)g(\varepsilon) = g(k)\lvert dk/d\varepsilon\rvert = (Vk^2/\pi^2)(m_e/\hbar^2 k). \blacksquare

At the Fermi energy: g(εF)=3N2εFg(\varepsilon_F) = \frac{3N}{2\varepsilon_F}.

The Fermi surface is the surface in k\mathbf{k}-space defined by ε(k)=εF\varepsilon(\mathbf{k}) = \varepsilon_F. For the free electron gas, this is a sphere of radius kFk_F. The shape of the Fermi surface Strongly influences transport properties (conductivity, Hall effect, cyclotron resonance).

In real metals, the periodic potential distorts the Fermi surface from a sphere. At the Brillouin Zone boundaries, band gaps open and the Fermi surface can develop “necks” (connecting to adjacent Zones) or become multiply connected. The topology of the Fermi surface determines whether a material Is a metal or insulator: a material is metallic if the Fermi surface crosses any Brillouin zone Boundary.

The number of electrons per atom determines the filling: 1 electron/atom (e.g., Na, Cu) gives a Nearly spherical Fermi surface well within the first BZ. 2 electrons/atom (e.g., Mg) nearly fills The first BZ and the Fermi surface contacts the zone boundary. 3—4 electrons/atom (e.g., Al, Pb) Produce complex multiply-connected Fermi surfaces.

5.3 Bloch”s Theorem

Theorem 5.1 (Bloch, 1928). The eigenstates of the one-electron Hamiltonian in a periodic Potential V(r+R)=V(r)V(\mathbf{r} + \mathbf{R}) = V(\mathbf{r}) can be written as:

ψnk(r)=eikrunk(r)\psi_{n\mathbf{k}}(\mathbf{r}) = e^{i\mathbf{k}\cdot\mathbf{r}} u_{n\mathbf{k}}(\mathbf{r})

Where unk(r)u_{n\mathbf{k}}(\mathbf{r}) has the periodicity of the lattice: unk(r+R)=unk(r)u_{n\mathbf{k}}(\mathbf{r} + \mathbf{R}) = u_{n\mathbf{k}}(\mathbf{r}).

Proof. The translation operators T^R\hat{T}_{\mathbf{R}} commute with the Hamiltonian H^=22m2+V(r)\hat{H} = -\frac{\hbar^2}{2m}\nabla^2 + V(\mathbf{r}) since VV is periodic. Therefore, the Eigenstates of H^\hat{H} can be chosen as simultaneous eigenstates of all T^R\hat{T}_{\mathbf{R}}:

T^Rψ(r)=ψ(r+R)=cRψ(r)\hat{T}_{\mathbf{R}}\psi(\mathbf{r}) = \psi(\mathbf{r} + \mathbf{R}) = c_{\mathbf{R}}\psi(\mathbf{r})

From the composition rule T^R1T^R2=T^R1+R2\hat{T}_{\mathbf{R}_1}\hat{T}_{\mathbf{R}_2} = \hat{T}_{\mathbf{R}_1 + \mathbf{R}_2}:

cR1+R2=cR1cR2c_{\mathbf{R}_1 + \mathbf{R}_2} = c_{\mathbf{R}_1} c_{\mathbf{R}_2}

The only solution of this functional equation is cR=eikRc_{\mathbf{R}} = e^{i\mathbf{k}\cdot\mathbf{R}}. Therefore ψ(r+R)=eikRψ(r)\psi(\mathbf{r} + \mathbf{R}) = e^{i\mathbf{k}\cdot\mathbf{R}}\psi(\mathbf{r})Which is Satisfied by ψ(r)=eikruk(r)\psi(\mathbf{r}) = e^{i\mathbf{k}\cdot\mathbf{r}}u_{\mathbf{k}}(\mathbf{r}) with uku_{\mathbf{k}} periodic. \blacksquare

Consequences:

  • k\mathbf{k} is defined only up to a reciprocal lattice vector: k\mathbf{k} and k+G\mathbf{k} + \mathbf{G} are equivalent.
  • The energy spectrum consists of bands εn(k)\varepsilon_n(\mathbf{k})Each labelled by a band index nn.
  • Band gaps appear between allowed energy bands.

5.4 Nearly Free Electron Model

Starting from the free electron model, a weak periodic potential V(r)=GVGeiGrV(\mathbf{r}) = \sum_{\mathbf{G}} V_{\mathbf{G}} e^{i\mathbf{G}\cdot\mathbf{r}} Opens gaps at the Brillouin zone boundaries where k=k+G\lvert\mathbf{k}\rvert = \lvert\mathbf{k} + \mathbf{G}\rvert (Bragg Condition).

At the zone boundary k=G/2\mathbf{k} = \mathbf{G}/2The gap is:

Δε=2VG\Delta\varepsilon = 2\lvert V_{\mathbf{G}}\rvert

Derivation. Near the zone boundary, the free electron states at k\mathbf{k} and kG\mathbf{k} - \mathbf{G} Are degenerate: εk0=εkG0\varepsilon_{\mathbf{k}}^0 = \varepsilon_{\mathbf{k} - \mathbf{G}}^0. Degenerate Perturbation theory gives:

det(εk0EVGVGεkG0E)=0\det\begin{pmatrix} \varepsilon_{\mathbf{k}}^0 - E & V_{\mathbf{G}} \\ V_{\mathbf{G}}^* & \varepsilon_{\mathbf{k} - \mathbf{G}}^0 - E \end{pmatrix} = 0

At k=G/2\mathbf{k} = \mathbf{G}/2: E=εG/20±VGE = \varepsilon_{\mathbf{G}/2}^0 \pm \lvert V_{\mathbf{G}}\rvertSo the gap is 2VG2\lvert V_{\mathbf{G}}\rvert. \blacksquare

5.5 Drude Model

The Drude model (1900) treats conduction electrons as a classical ideal gas scattering off Static ions with a mean free time τ\tau (relaxation time).

Equation of motion. Under an electric field E\mathbf{E}:

medvdt=eEmevτm_e\frac{d\mathbf{v}}{dt} = -e\mathbf{E} - \frac{m_e\mathbf{v}}{\tau}

The second term represents a frictional drag with characteristic time τ\tau.

DC conductivity. In steady state (dv/dt=0d\mathbf{v}/dt = 0): vd=eτmeE\mathbf{v}_d = -\frac{e\tau}{m_e}\mathbf{E}. The current density: J=nevd=ne2τmeE\mathbf{J} = -ne\mathbf{v}_d = \frac{ne^2\tau}{m_e}\mathbf{E}.

σ=ne2τme\sigma = \frac{ne^2\tau}{m_e}

AC conductivity. For E(t)=E0eiωt\mathbf{E}(t) = \mathbf{E}_0\,e^{-i\omega t}The Drude model gives:

σ(ω)=ne2τ/me1iωτ=σ01iωτ\sigma(\omega) = \frac{ne^2\tau/m_e}{1 - i\omega\tau} = \frac{\sigma_0}{1 - i\omega\tau}

The real part Re[σ(ω)]=σ01+ω2τ2\mathrm{Re}[\sigma(\omega)] = \frac{\sigma_0}{1 + \omega^2\tau^2} describes absorption, Peaking at ω=0\omega = 0 (the Drude peak). This explains the metallic reflectivity in the infrared.

Hall effect. With B=Bz^\mathbf{B} = B\hat{z} applied, the steady-state equation becomes:

eEmevτev×B=0-e\mathbf{E} - \frac{m_e\mathbf{v}}{\tau} - e\mathbf{v} \times \mathbf{B} = 0

For current J=Jxx^\mathbf{J} = J_x\hat{x}A transverse field EyE_y develops:

RH=EyJxB=1neR_H = \frac{E_y}{J_x B} = -\frac{1}{ne}

This provides a direct measurement of the carrier density nn.

Successes: Ohm”s law (J=σE\mathbf{J} = \sigma\mathbf{E}), Wiedemann—Franz law (κ/σT=π2kB23e2\kappa/\sigma T = \frac{\pi^2 k_B^2}{3e^2}), Hall effect.

Failures: Predicts χT1\chi \propto T^{-1} (Curie law) for magnetic susceptibility, but real Metals have nearly temperature-independent Pauli paramagnetism. Predicts CV=32nkBC_V = \frac{3}{2}nk_B But experiments give CV32nkBC_V \ll \frac{3}{2}nk_B at room temperature.

5.6 Sommerfeld Model

The Sommerfeld model (1928) corrects the Drude model by treating electrons as a Fermi gas Obeying Fermi—Dirac …/4-statistics-and-probability/2_statistics:

f(ε)=1e(εμ)/kBT+1f(\varepsilon) = \frac{1}{e^{(\varepsilon - \mu)/k_B T} + 1}

At T=0T = 0The chemical potential equals the Fermi energy: μ(0)=εF\mu(0) = \varepsilon_F. At finite TT:

μ(T)=εF[1π212(kBTεF)2+]\mu(T) = \varepsilon_F\left[1 - \frac{\pi^2}{12}\left(\frac{k_B T}{\varepsilon_F}\right)^2 + \cdots\right]

Since εF/kB104\varepsilon_F/k_B \sim 10^4 K for metals, the correction at room temperature is negligible: The chemical potential is essentially constant.

Electronic specific heat. By the Sommerfeld expansion:

Ce=π23kB2g(εF)T=γTC_e = \frac{\pi^2}{3}k_B^2\,g(\varepsilon_F)\,T = \gamma T

Where γ=π22NkB2εF\gamma = \frac{\pi^2}{2}\frac{Nk_B^2}{\varepsilon_F}. At room temperature, only electrons within kBT\sim k_B T of εF\varepsilon_F can be thermally excited, which is a tiny fraction T/TF1/100\sim T/T_F \sim 1/100 of the total. This explains why Ce32NkBC_e \ll \frac{3}{2}Nk_B.

Pauli paramagnetism. The spin susceptibility of a degenerate electron gas:

χP=μ0μB2g(εF)=3μ0μB2N2εF\chi_P = \mu_0\mu_B^2\,g(\varepsilon_F) = \frac{3\mu_0\mu_B^2 N}{2\varepsilon_F}

This is independent of TT (up to corrections of order (T/TF)2(T/T_F)^2), in contrast to the Curie law χ1/T\chi \propto 1/T of the Drude model.

Derivation: Sommerfeld Expansion

To compute thermal averages at low TTWe integrate h(ε)f(ε)h(\varepsilon) f(\varepsilon) where f(ε)=1/(eβ(εμ)+1)f(\varepsilon) = 1/(e^{\beta(\varepsilon - \mu)} + 1) is the Fermi—Dirac distribution and h(ε)h(\varepsilon) Is any smooth function (e.g., density of states times energy).

Define H(ε)=0εh(ε)dεH(\varepsilon) = \int_0^\varepsilon h(\varepsilon')\,d\varepsilon'. Then:

I=0h(ε)f(ε)dε=0dHdεfdε=[Hf]0+0H(ε)(fε)dεI = \int_0^\infty h(\varepsilon)f(\varepsilon)\,d\varepsilon = \int_0^\infty \frac{dH}{d\varepsilon}\,f\,d\varepsilon = [Hf]_0^\infty + \int_0^\infty H(\varepsilon)\left(-\frac{\partial f}{\partial \varepsilon}\right)d\varepsilon

Since f(0)1f(0) \approx 1 and f()=0f(\infty) = 0And f/ε-\partial f/\partial \varepsilon is sharply peaked At ε=μ\varepsilon = \mu with width kBT\sim k_B TWe expand H(ε)H(\varepsilon) about μ\mu:

I=0μh(ε)dε+π26(kBT)2h(μ)+I = \int_0^\mu h(\varepsilon)\,d\varepsilon + \frac{\pi^2}{6}(k_B T)^2 h'(\mu) + \cdots

For the total energy with h(ε)=εg(ε)h(\varepsilon) = \varepsilon\,g(\varepsilon):

E=0μ0εg(ε)dε+π26(kBT)2ddε[εg(ε)]ε=μ0+E = \int_0^{\mu_0} \varepsilon\,g(\varepsilon)\,d\varepsilon + \frac{\pi^2}{6}(k_B T)^2 \frac{d}{d\varepsilon}[\varepsilon g(\varepsilon)]_{\varepsilon = \mu_0} + \cdots

Differentiating with respect to TT gives the specific heat CV=π23kB2g(εF)TC_V = \frac{\pi^2}{3}k_B^2\,g(\varepsilon_F)\,T. \blacksquare

Worked Example: Fermi Energy of Sodium

Sodium has n=2.65×1028 m3n = 2.65 \times 10^{28}\ \mathrm{m}^{-3} conduction electrons (one per atom, BCC structure).

kF=(3π2n)1/3=(3π2×2.65×1028)1/3=(7.85×1029)1/3=9.23×109 m1k_F = (3\pi^2 n)^{1/3} = (3\pi^2 \times 2.65 \times 10^{28})^{1/3} = (7.85 \times 10^{29})^{1/3} = 9.23 \times 10^9\ \mathrm{m}^{-1}

εF=2kF22me=(1.055×1034)2×(9.23×109)22×9.11×1031=9.48×10581.82×1030=5.21×1019 J=3.25 eV\varepsilon_F = \frac{\hbar^2 k_F^2}{2m_e} = \frac{(1.055 \times 10^{-34})^2 \times (9.23 \times 10^9)^2}{2 \times 9.11 \times 10^{-31}} = \frac{9.48 \times 10^{-58}}{1.82 \times 10^{-30}} = 5.21 \times 10^{-19}\ \mathrm{J} = 3.25\ \mathrm{eV}

TF=εFkB=5.21×10191.381×1023=3.77×104 KT_F = \frac{\varepsilon_F}{k_B} = \frac{5.21 \times 10^{-19}}{1.381 \times 10^{-23}} = 3.77 \times 10^4\ \mathrm{K}

vF=kFme=1.055×1034×9.23×1099.11×1031=1.07×106 m/sv_F = \frac{\hbar k_F}{m_e} = \frac{1.055 \times 10^{-34} \times 9.23 \times 10^9}{9.11 \times 10^{-31}} = 1.07 \times 10^6\ \mathrm{m}/s

The electronic specific heat coefficient: γ=π22nkB2εF=π2×2.65×1028×(1.381×1023)22×5.21×1019=1.38×103 J/(m3K2)\gamma = \frac{\pi^2}{2}\frac{nk_B^2}{\varepsilon_F} = \frac{\pi^2 \times 2.65 \times 10^{28} \times (1.381 \times 10^{-23})^2}{2 \times 5.21 \times 10^{-19}} = 1.38 \times 10^3\ \mathrm{J}/(m^3\cdot K^2)

5.7 Tight-Binding Model

The tight-binding model starts from isolated atomic orbitals and treats the overlap between Neighbours as a perturbation. For a 1D chain with lattice constant aa and a single ss-orbital Of energy ε0\varepsilon_0:

ψk(r)=1Nneiknaϕ(rna)\psi_k(r) = \frac{1}{\sqrt{N}}\sum_n e^{ikna}\,\phi(r - na)

Where ϕ(rna)\phi(r - na) is the atomic orbital centred at site nn.

Dispersion relation (nearest-neighbour approximation):

ε(k)=ε02tcos(ka)\varepsilon(k) = \varepsilon_0 - 2t\cos(ka)

Where t=ϕ(rna)H^ϕ(r(n+1)a)drt = -\int \phi^*(r - na)\,\hat{H}\,\phi(r - (n+1)a)\,dr is the hopping integral (t>0t > 0 for typical ss-orbitals).

Key features:

  • Band width: W=4tW = 4t.
  • Minimum at k=0k = 0: εmin=ε02t\varepsilon_{\min} = \varepsilon_0 - 2t.
  • Maximum at k=±π/ak = \pm\pi/a: εmax=ε0+2t\varepsilon_{\max} = \varepsilon_0 + 2t.
  • Effective mass at band bottom: m=2/(2ta2)m^* = \hbar^2/(2ta^2).

Extension to 3D: For a simple cubic lattice with nearest-neighbour hopping:

ε(k)=ε02t(coskxa+coskya+coskza)\varepsilon(\mathbf{k}) = \varepsilon_0 - 2t(\cos k_x a + \cos k_y a + \cos k_z a)

The band width is W=12tW = 12t and the density of states develops a van Hove singularity at ε=ε0\varepsilon = \varepsilon_0.

Worked Example: Tight-Binding Band Structure of Graphene

Graphene has a honeycomb lattice with two carbon atoms per unit cell. Using pzp_z orbitals with Nearest-neighbour hopping t2.8t \approx 2.8 eV, the tight-binding Hamiltonian gives:

ε±(k)=±t1+eika1+eika2\varepsilon_{\pm}(\mathbf{k}) = \pm t\left\lvert 1 + e^{i\mathbf{k}\cdot\mathbf{a}_1} + e^{i\mathbf{k}\cdot\mathbf{a}_2}\right\rvert

Where a1\mathbf{a}_1 and a2\mathbf{a}_2 are the primitive vectors of the hexagonal lattice.

The two bands touch at the Dirac points K\mathbf{K} and K\mathbf{K}' in the Brillouin zone. Near these points, expanding to linear order:

ε(q)=±vFq\varepsilon(\mathbf{q}) = \pm \hbar v_F \lvert\mathbf{q}\rvert

Where vF=32ta106v_F = \frac{\sqrt{3}}{2}\frac{ta}{\hbar} \approx 10^6 m/s and q=kK\mathbf{q} = \mathbf{k} - \mathbf{K}.

This linear (Dirac-like) dispersion means graphene has zero effective mass and a density of states g(ε)εg(\varepsilon) \propto \lvert\varepsilon\rvert (linear in energy), unlike the ε\sqrt{\varepsilon} Dependence of a parabolic band.

5.8 Effective Mass

Near a band extremum at k0\mathbf{k}_0The energy can be expanded:

ε(k)=ε0+22ij(m1)ij(kik0,i)(kjk0,j)\varepsilon(\mathbf{k}) = \varepsilon_0 + \frac{\hbar^2}{2}\sum_{ij}(m^{-1})_{ij}(k_i - k_{0,i})(k_j - k_{0,j})

The effective mass tensor (m1)ij=122εkikj(m^{-1})_{ij} = \frac{1}{\hbar^2}\frac{\partial^2 \varepsilon}{\partial k_i \partial k_j} Determines the response to external fields. For isotropic bands, m=2/(d2ε/dk2)m^* = \hbar^2/(d^2\varepsilon/dk^2).

A large effective mass means a flat band (small group velocity). A small effective mass means a Steep band (high mobility).

The effective mass can be negative near a band maximum (holes). Cyclotron resonance experiments Measure mm^* directly: the resonance frequency is ωc=eB/m\omega_c = eB/m^*.

:::caution Common Pitfall The effective mass is a tensor quantity . For crystals with cubic symmetry, it reduces to A scalar, but for anisotropic crystals (e.g., graphite, silicon), different effective masses apply Along different crystallographic directions. Always check the crystal symmetry before assuming mm^* is a scalar.

5.9 Band Structure Calculations

Modern band structure calculations are based on density functional theory (DFT), formulated by Hohenberg, Kohn, and Sham (1964—1965).

Hohenberg—Kohn theorems. (1) The ground-state energy of a many-electron system is a unique Functional of the electron density n(r)n(\mathbf{r}). (2) The correct ground-state density minimises This functional.

Kohn—Sham equations. The interacting system is mapped to a fictitious system of non-interacting Electrons in an effective potential:

\left[-\frac{\hbar^2}{2m}\nabla^2 + V_{\mathrm{eff}(\mathbf{r})\right]\psi_i(\mathbf{r}) = \varepsilon_i\psi_i(\mathbf{r})}

Where Veff=Vext+VH[n]+Vxc[n]V_{\mathrm{eff} = V_{\mathrm{ext} + V_H[n] + V_{\mathrm{xc}[n]}}}. Here VextV_{\mathrm{ext}} is the External (ionic) potential, VHV_H is the Hartree (classical Coulomb) potential, and VxcV_{\mathrm{xc}} Is the exchange-correlation potential.

The electron density is n(r)=iψi(r)2n(\mathbf{r}) = \sum_i \lvert\psi_i(\mathbf{r})\rvert^2 (summing over occupied States). The Kohn—Sham equations are solved self-consistently.

Common approximations for VxcV_{\mathrm{xc}}:

  • Local density approximation (LDA): Vxc(r)=Vxchom(n(r))V_{\mathrm{xc}(\mathbf{r}) = V_{\mathrm{xc}^{\mathrm{hom}(n(\mathbf{r}))}}} using the exchange-correlation energy of a homogeneous electron gas. Good for simple metals but tends to underestimate band gaps.
  • Generalised gradient approximation (GGA): Includes the density gradient n(r)\nabla n(\mathbf{r})Improving accuracy for structural properties and band gaps.
  • Hybrid functionals (e.g., HSE06): Mix a fraction of exact Hartree—Fock exchange with DFT exchange, giving improved band gaps at higher computational cost.

DFT accurately predicts structural properties (lattice constants, elastic constants, phonon Frequencies within a few percent) but is less reliable for band gaps (LDA underestimates By 30—50%) and strongly correlated systems (e.g., transition metal oxides).

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