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The nearly-free-electron model is controlled perturbation theory around free plane waves in a weak periodic potential. Away from free-electron degeneracies, the potential produces small energy shifts and weak reciprocal-lattice satellites. At a Bragg plane, however, two or more plane waves are degenerate, ordinary perturbation theory fails, and even an arbitrarily weak Fourier component can split the degeneracy at first order.

For an isolated two-wave crossing, the leading direct gap is

ΔG=2∣VG∣,\Delta_{\mathbf G} = 2|V_{\mathbf G}|,

where VGV_{\mathbf G} is the Fourier coefficient of the periodic potential at the reciprocal vector connecting the two waves. This compact result explains why zone boundaries are special, but it must be read with its assumptions: the crossing must be isolated from other free branches, omitted couplings must be perturbative, and a local avoided crossing is not automatically a global insulating gap.

Bloch’s Theorem is exact and supplies the crystal-momentum sectors. We now approximate the Hamiltonian within those sectors, keeping the waves that become resonant at a Bragg plane and estimating the effects of the others.

Required background. Bloch’s Theorem supplies the exact crystal-momentum sectors, Brillouin Zones supplies zone-boundary geometry and folding conventions, and Degenerate Perturbation Theory supplies the avoided-crossing calculation at a Bragg plane.

Consider

H=H0+V,H0=p22m,H = H_0+V, \qquad H_0 = \frac{\mathbf p^2}{2m},

with a real lattice-periodic potential,

V(r+R)=V(r).V(\mathbf r+\mathbf R) = V(\mathbf r).

Expand it in reciprocal vectors:

V(r)=∑GVGeiG⋅r,V(\mathbf r) = \sum_{\mathbf G} V_{\mathbf G} e^{i\mathbf G\cdot\mathbf r},

where

VG=1Ωc∫cellddr V(r)e−iG⋅r.V_{\mathbf G} = \frac{1}{\Omega_c} \int_{\mathrm{cell}} d^dr\, V(\mathbf r) e^{-i\mathbf G\cdot\mathbf r}.

Reality implies

V−G=VG∗.V_{-\mathbf G} = V_{\mathbf G}^{\ast}.

The average V0V_{\mathbf0} shifts every energy equally and can be absorbed into the energy origin. The nonzero coefficients scatter a plane wave with wavevector q\mathbf q into waves at

q−G.\mathbf q-\mathbf G.

“Nearly free” means that the relevant VGV_{\mathbf G} are small compared with the energy separations to plane-wave branches excluded from a chosen perturbative subspace. It does not mean that every microscopic ionic potential is weak at every point. In practical electronic-structure reasoning, screening and pseudopotentials can make the effective potential seen by valence electrons much smoother than the bare core potential.

For NcN_c primitive cells with Born–von Karman boundary conditions, free eigenstates are normalized plane waves,

⟨r∣q⟩=1Veiq⋅r,V=NcΩc,\langle\mathbf r|\mathbf q\rangle = \frac{1}{\sqrt V} e^{i\mathbf q\cdot\mathbf r}, \qquad V=N_c\Omega_c,

with energies

εq=ℏ2∣q∣22m.\varepsilon_{\mathbf q} = \frac{\hbar^2|\mathbf q|^2}{2m}.

Choose k\mathbf k in one Brillouin zone. Every allowed plane wave can be written uniquely as

q=k+G.\mathbf q = \mathbf k+\mathbf G.

At fixed k\mathbf k, the free basis is therefore

{∣k+G⟩}G∈Λ∗,\left\{ |\mathbf k+\mathbf G\rangle \right\}_{\mathbf G\in\Lambda^\ast},

with folded branches

εG(k)=ℏ22m∣k+G∣2.\varepsilon_{\mathbf G}(\mathbf k) = \frac{\hbar^2}{2m} |\mathbf k+\mathbf G|^2.

Folding these parabolas into one zone is only a relabeling of the free spectrum. It creates branch crossings on a plot but does not open a gap. Gaps appear only after the periodic potential couples crossing branches.

A Bloch state at fixed k\mathbf k has the plane-wave expansion

ψnk(r)=∑Gcnk(G)ei(k+G)⋅r.\psi_{n\mathbf k}(\mathbf r) = \sum_{\mathbf G} c_{n\mathbf k}(\mathbf G) e^{i(\mathbf k+\mathbf G)\cdot\mathbf r}.

The matrix element of the potential is

⟨k+G∣V∣k+G′⟩=VG−G′.\langle \mathbf k+\mathbf G | V | \mathbf k+\mathbf G' \rangle = V_{\mathbf G-\mathbf G'}.

Substitution into the Schrödinger equation gives the central equation

∑G′[εG(k)δGG′+VG−G′]cnk(G′)=En(k)cnk(G).\sum_{\mathbf G'} \left[ \varepsilon_{\mathbf G}(\mathbf k) \delta_{\mathbf G\mathbf G'} + V_{\mathbf G-\mathbf G'} \right] c_{n\mathbf k}(\mathbf G') = E_n(\mathbf k) c_{n\mathbf k}(\mathbf G).

Equivalently,

[εG(k)−En(k)]cnk(G)+∑G′VG−G′cnk(G′)=0.\left[ \varepsilon_{\mathbf G}(\mathbf k) -E_n(\mathbf k) \right] c_{n\mathbf k}(\mathbf G) + \sum_{\mathbf G'} V_{\mathbf G-\mathbf G'} c_{n\mathbf k}(\mathbf G') = 0.

This is an infinite matrix eigenproblem within one Bloch sector. A plane-wave calculation truncates the reciprocal basis at a kinetic-energy cutoff; the nearly-free approximation instead keeps only the resonant branches analytically and treats the rest perturbatively.

Suppose the free plane wave ∣q⟩|\mathbf q\rangle is separated in energy from every ∣q−G⟩|\mathbf q-\mathbf G\rangle coupled appreciably by the potential. Nondegenerate perturbation theory gives

E(q)=εq+V0+∑G≠0∣VG∣2εq−εq−G+O(V3).E(\mathbf q) = \varepsilon_{\mathbf q} + V_{\mathbf0} + \sum_{\mathbf G\ne\mathbf0} \frac{|V_{\mathbf G}|^2} {\varepsilon_{\mathbf q}-\varepsilon_{\mathbf q-\mathbf G}} + O(V^3).

The first-order correction is only the spatial average V0V_{\mathbf0}. The nonuniform potential changes a nondegenerate free energy first at second order, although it changes the eigenvector at first order.

The expansion fails when a denominator becomes small:

εq≈εq−G.\varepsilon_{\mathbf q} \approx \varepsilon_{\mathbf q-\mathbf G}.

This is not a technical nuisance to be ignored. It identifies the Bragg planes where a qualitatively new two-wave or multiwave problem must be solved.

Free waves k\mathbf k and k−G\mathbf k-\mathbf G are degenerate when

ℏ2∣k∣22m=ℏ2∣k−G∣22m.\frac{\hbar^2|\mathbf k|^2}{2m} = \frac{\hbar^2|\mathbf k-\mathbf G|^2}{2m}.

Canceling common terms yields

k⋅G=∣G∣22.\mathbf k\cdot\mathbf G = \frac{|\mathbf G|^2}{2}.

This is the perpendicular-bisector equation for a reciprocal-lattice vector. The nearest such planes are exactly the faces used to construct the first Brillouin zone.

The same condition is the elastic Bragg-scattering condition. The periodic potential can transfer reciprocal momentum ℏG\hbar\mathbf G without changing the free kinetic energy, so the incident and Bragg-reflected waves mix coherently.

Near an isolated Bragg plane, retain

∣k⟩and∣k−G⟩.|\mathbf k\rangle \quad\text{and}\quad |\mathbf k-\mathbf G\rangle.

To first order in the weak potential, the effective Hamiltonian is

Heff=(εk+V0VGVG∗εk−G+V0).H_{\mathrm{eff}} = \begin{pmatrix} \varepsilon_{\mathbf k}+V_{\mathbf0} & V_{\mathbf G} \\ V_{\mathbf G}^{\ast} & \varepsilon_{\mathbf k-\mathbf G}+V_{\mathbf0} \end{pmatrix}.

Its eigenvalues are

E±(k)=V0+εk+εk−G2±(εk−εk−G2)2+∣VG∣2.E_{\pm}(\mathbf k) = V_{\mathbf0} + \frac{ \varepsilon_{\mathbf k} + \varepsilon_{\mathbf k-\mathbf G} }{2} \pm \sqrt{ \left( \frac{ \varepsilon_{\mathbf k} - \varepsilon_{\mathbf k-\mathbf G} }{2} \right)^2 + |V_{\mathbf G}|^2 }.

At exact degeneracy,

E±=εB+V0±∣VG∣,E_{\pm} = \varepsilon_{\mathrm B} + V_{\mathbf0} \pm |V_{\mathbf G}|,

so the leading avoided-crossing gap is

ΔG=E+−E−=2∣VG∣.\Delta_{\mathbf G} = E_+-E_- = 2|V_{\mathbf G}|.

Corrections from omitted plane waves begin at higher order when those waves remain well separated. If several free branches are degenerate, the two-state formula is insufficient and the full degenerate block must be diagonalized.

Two folded free-electron parabolas crossing at a Bragg plane and the avoided crossing produced by a weak periodic potential, with gap two times the magnitude of V sub G.

Folding alone produces a crossing between εk\varepsilon_{\mathbf k} and εk−G\varepsilon_{\mathbf k-\mathbf G}. The Fourier coefficient VGV_{\mathbf G} couples the degenerate waves and replaces the crossing by two smooth branches separated by 2∣VG∣2|V_{\mathbf G}| at the Bragg plane. Here κ\kappa measures displacement normal to the plane.

For a lattice spacing aa, take

G=2πa,k=G2+κ.G = \frac{2\pi}{a}, \qquad k = \frac{G}{2}+\kappa.

The coupled wavevectors are

k=G2+κ,k−G=−G2+κ.k = \frac{G}{2}+\kappa, \qquad k-G = -\frac{G}{2}+\kappa.

Their average free energy and half-difference are

εk+εk−G2=ℏ2G28m+ℏ2κ22m,\frac{ \varepsilon_k+\varepsilon_{k-G} }{2} = \frac{\hbar^2G^2}{8m} + \frac{\hbar^2\kappa^2}{2m}, εk−εk−G2=ℏ2Gκ2m.\frac{ \varepsilon_k-\varepsilon_{k-G} }{2} = \frac{\hbar^2G\kappa}{2m}.

The two-wave dispersion is therefore

E±(κ)=V0+ℏ2G28m+ℏ2κ22m±(ℏ2Gκ2m)2+∣VG∣2.E_{\pm}(\kappa) = V_0 + \frac{\hbar^2G^2}{8m} + \frac{\hbar^2\kappa^2}{2m} \pm \sqrt{ \left( \frac{\hbar^2G\kappa}{2m} \right)^2 + |V_G|^2 }.

Far enough from the boundary that

∣ℏ2Gκ2m∣≫∣VG∣,\left| \frac{\hbar^2G\kappa}{2m} \right| \gg |V_G|,

the branches approach the folded free parabolas. Inside the mixing region, the eigenstates contain comparable right- and left-moving components and the free crossing is rounded.

Write

VG=∣VG∣eiϕ.V_G = |V_G|e^{i\phi}.

At k=G/2k=G/2, the coefficient vectors have unit norm. The corresponding functions, with unit cell-average density, may be chosen as

ψ±(x)=12[eiGx/2±e−iϕe−iGx/2].\psi_{\pm}(x) = \frac{1}{\sqrt2} \left[ e^{iGx/2} \pm e^{-i\phi}e^{-iGx/2} \right].

Their densities are

∣ψ±(x)∣2=1±cos⁡(Gx+ϕ).|\psi_{\pm}(x)|^2 = 1 \pm \cos(Gx+\phi).

The resonant part of the potential is

VGeiGx+V−Ge−iGx=2∣VG∣cos⁡(Gx+ϕ).V_Ge^{iGx} + V_{-G}e^{-iGx} = 2|V_G| \cos(Gx+\phi).

For a unit-normalized wavefunction in a finite chain of length LL, divide the displayed function by L\sqrt L. The upper state concentrates density near maxima of this harmonic, while the lower state concentrates near its minima. Translating the coordinate origin changes ϕ\phi and shifts both patterns, but it cannot change the energies or the gap 2∣VG∣2|V_G|.

The safest rule is to compute the Fourier coefficient before quoting a gap. If

V(x)=2Ucos⁡(Gx),V(x) = 2U\cos(Gx),

then

VG=V−G=U,V_G = V_{-G} = U,

and

ΔG=2∣U∣.\Delta_G = 2|U|.

If another author writes

V(x)=Ucos⁡(Gx),V(x) = U\cos(Gx),

then VG=U/2V_G=U/2 and the gap is ∣U∣|U|. Both statements are the same physics with different definitions of the cosine amplitude. Writing “the gap equals twice the potential” without defining the Fourier convention is ambiguous.

The reduced, extended and repeated zone schemes display the same states in different ways. Folding labels the uncoupled branches; a nonzero matrix element changes their eigenvalues. Near the avoided crossing, the eigenvectors continuously exchange their dominant plane-wave character. Consequently, following the most intense plane-wave component can jump between energy-ordered bands.

On a generic face of a Brillouin zone, the two-wave derivation applies to motion normal to that face. Momentum parallel to the face remains continuous, so the avoided crossing forms a gapped sheet rather than an isolated point.

At an edge or corner, several reciprocal vectors can generate simultaneous degeneracies. If the resonant plane waves are

{∣k+G1⟩,…,∣k+GM⟩},\left\{ |\mathbf k+\mathbf G_1\rangle, \ldots, |\mathbf k+\mathbf G_M\rangle \right\},

one must diagonalize the M×MM\times M matrix

[Hdeg(k)]ij=εk+Giδij+VGi−Gj.\left[ H_{\mathrm{deg}}(\mathbf k) \right]_{ij} = \varepsilon_{\mathbf k+\mathbf G_i} \delta_{ij} + V_{\mathbf G_i-\mathbf G_j}.

Point-group symmetry constrains this matrix and can protect residual degeneracies. A geometrical free-electron crossing does not guarantee a first-order gap: the required VGV_{\mathbf G} may vanish by symmetry or motif interference.

2∣VG∣2|V_{\mathbf G}| is a local direct splitting between two branches at a particular Bragg plane. A band insulator at zero temperature requires a global gap at the chosen integer filling: all occupied bands must be separated in energy from all unoccupied bands throughout the zone. This criterion concerns clean independent-electron band insulation; disorder and interactions can produce other insulating mechanisms. In two and three dimensions, different folded free branches often overlap in energy even though each individual avoided crossing is nonzero.

Let

V(x)=2Ucos⁡(2πxa).V(x) = 2U\cos\left(\frac{2\pi x}{a}\right).

Only

V±2π/a=UV_{\pm 2\pi/a} = U

are nonzero apart from the average. At the first-zone boundaries k=±π/ak=\pm\pi/a, the leading gap is 2∣U∣2|U|. The same harmonic also couples other pairs of plane waves separated by 2π/a2\pi/a, but only resonant pairs acquire a first-order splitting.

For

V(x)=2Ucos⁡[G(x−x0)],V(x) = 2U \cos \left[ G(x-x_0) \right],

the coefficient is

VG=Ue−iGx0.V_G = Ue^{-iGx_0}.

The shift changes the phase of the coupling and the position of the standing-wave nodes. Since

∣VG∣=∣U∣,|V_G| = |U|,

the band energies and gap are independent of the arbitrary origin.

Take

V(x,y)=2Uxcos⁡(Gxx)+2Uycos⁡(Gyy).V(x,y) = 2U_x\cos(G_xx) + 2U_y\cos(G_yy).

At the Bragg plane kx=Gx/2k_x=G_x/2 away from a zone corner, the relevant pair differs by Gxx^G_x\hat{\mathbf x} and the leading splitting is 2∣Ux∣2|U_x|. Similarly, the ky=Gy/2k_y=G_y/2 face has splitting 2∣Uy∣2|U_y|.

At their intersection, four free plane waves are degenerate. For this separable potential the leading block is

Hcorner=εBI4+Uxσx⊗I2+UyI2⊗σx,H_{\rm corner}=\varepsilon_{\rm B}I_4 +U_x\sigma_x\otimes I_2+U_y I_2\otimes\sigma_x,

with energies εB±Ux±Uy\varepsilon_{\rm B}\pm U_x\pm U_y for real Ux,UyU_x,U_y. If Ux=Uy=UU_x=U_y=U, the shifts are −2U,0,0,2U-2U,0,0,2U: a doublet remains in the middle. A Fourier harmonic coupling both directions generally destroys this separability and requires the full four-state calculation.

Let PP project onto the retained resonant plane waves and Q=1−PQ=1-P. The approximation is controlled when matrix elements coupling PP to QQ are small compared with the corresponding free-energy separations:

∣⟨p∣V∣q⟩∣∣Ep(0)−Eq(0)∣≪1\frac{ |\langle p|V|q\rangle| }{ |E_p^{(0)}-E_q^{(0)}| } \ll 1

for the omitted states that matter. Many individually small terms can nevertheless accumulate. A useful state-specific estimate of omitted weight is

wQ≃∑q∈Q∣⟨q∣V∣p⟩∣2∣Ep(0)−Eq(0)∣2≪1.w_Q\simeq\sum_{q\in Q} \frac{|\langle q|V|p\rangle|^2}{|E_p^{(0)}-E_q^{(0)}|^2}\ll1.

For a retained block, the corresponding condition involves the norm of the coupling times the omitted-space resolvent. Convergence with a larger plane-wave cutoff tests the cumulative effect. Near a multiwave degeneracy, enlarge PP rather than forcing a two-state treatment.

When many Fourier components mix strongly, a low-order nearly-free expansion loses quantitative accuracy. A larger plane-wave diagonalization remains valid as a numerical representation, while a tight-binding or Wannier description may be more economical for localized bands. These are different approximations to the same Bloch problem, not competing versions of Bloch’s theorem.

Bare ionic potentials are singular and core wavefunctions oscillate strongly. Nearly-free reasoning is most natural for delocalized valence states after core physics has been incorporated into an effective potential. Orthogonality to core states and nonlocal pseudopotentials can be essential even when the resulting valence dispersion looks free-electron-like.

The elementary model is a one-particle Hamiltonian. Electron–electron interactions can renormalize dispersions, transfer spectral weight, and produce finite lifetimes or entirely new phases. Disorder broadens crystal momentum and can obscure small gaps. A fitted nearly-free band should therefore be identified as a one-particle or quasiparticle description, not as the exact many-body spectrum.

For real VG>0V_G>0 at k=G/2k=G/2, show that the symmetric standing wave is the upper state and the antisymmetric standing wave is the lower state. How does the answer change when VG<0V_G<0?

Solution

The two-state matrix at the boundary is

Heff=(εBVGVGεB).H_{\mathrm{eff}} = \begin{pmatrix} \varepsilon_{\mathrm B} & V_G \\ V_G & \varepsilon_{\mathrm B} \end{pmatrix}.

For VG>0V_G>0, the vector (1,1)/2(1,1)/\sqrt2 has energy εB+VG\varepsilon_{\mathrm B}+V_G and produces

ψ+(x)∝cos⁡(Gx/2).\psi_+(x) \propto \cos(Gx/2).

The vector (1,−1)/2(1,-1)/\sqrt2 has energy εB−VG\varepsilon_{\mathrm B}-V_G and produces

ψ−(x)∝sin⁡(Gx/2)\psi_-(x) \propto \sin(Gx/2)

up to an overall phase. When VG<0V_G<0, the eigenvectors are the same but their energy ordering reverses. The lower state always places more density near minima of the resonant potential harmonic.

Use the one-dimensional formula for E±(κ)E_{\pm}(\kappa) to show that far from the mixing region the two eigenvalues approach εk+V0\varepsilon_k+V_0 and εk−G+V0\varepsilon_{k-G}+V_0.

Solution

Define

δ(κ)=εk−εk−G2=ℏ2Gκ2m.\delta(\kappa) = \frac{ \varepsilon_k-\varepsilon_{k-G} }{2} = \frac{\hbar^2G\kappa}{2m}.

When ∣δ∣≫∣VG∣|\delta|\gg|V_G|,

δ2+∣VG∣2=∣δ∣+O(∣VG∣2∣δ∣).\sqrt{\delta^2+|V_G|^2} = |\delta| + O\left( \frac{|V_G|^2}{|\delta|} \right).

The two eigenvalues become the average free energy plus or minus ∣δ∣|\delta|. Those are the larger and smaller of εk\varepsilon_k and εk−G\varepsilon_{k-G}, with only second-order corrections. Their ordering swaps as κ\kappa crosses zero, which is why the coupled branches avoid rather than pass through one another.

Translate the coordinate origin by r0\mathbf r_0. Show how VGV_{\mathbf G} transforms and prove that the two-wave energies are unchanged.

Solution

With the new coordinate r′=r−r0\mathbf r'=\mathbf r-\mathbf r_0,

V(r′+r0)=∑GVGeiG⋅r0eiG⋅r′.V(\mathbf r'+\mathbf r_0) = \sum_{\mathbf G} V_{\mathbf G} e^{i\mathbf G\cdot\mathbf r_0} e^{i\mathbf G\cdot\mathbf r'}.

Thus

VG′=eiG⋅r0VG.V_{\mathbf G}' = e^{i\mathbf G\cdot\mathbf r_0} V_{\mathbf G}.

The phase changes but

∣VG′∣=∣VG∣.|V_{\mathbf G}'| = |V_{\mathbf G}|.

Since the eigenvalues depend on the coupling through ∣VG∣2|V_{\mathbf G}|^2, the dispersion and gap are origin independent. The eigenvector phases transform so that the real-space state is described consistently.

Exercise 4: a gap without the direct Fourier harmonic

Section titled “Exercise 4: a gap without the direct Fourier harmonic”

Take V(x)=2Ucos⁡(Gx)V(x)=2U\cos(Gx) with real ∣U∣≪EG=ℏ2G2/(2m)|U|\ll E_G=\hbar^2G^2/(2m). At reduced momentum k=0k=0, the free waves ∣+G⟩|+G\rangle and ∣−G⟩|-G\rangle are degenerate. Although V2G=0V_{2G}=0, show that a gap opens at second order. Include the common diagonal energy shift.

Solution

The path +G→0→−G+G\to0\to-G has two matrix elements UU and denominator EG−0E_G-0. It produces the off-diagonal element U2/EGU^2/E_G. For each diagonal entry, intermediate waves at 0 and ±2G\pm2G give

δE=U2EG+U2EG−4EG=2U23EG.\delta E=\frac{U^2}{E_G}+\frac{U^2}{E_G-4E_G} =\frac{2U^2}{3E_G}.

Thus

Heff=(EG+2U23EG)I2+U2EGσx+O(U4/EG3),H_{\rm eff}=\left(E_G+\frac{2U^2}{3E_G}\right)I_2 +\frac{U^2}{E_G}\sigma_x+O(U^4/E_G^3),

and the leading gap is 2U2/EG2U^2/E_G. Each scattering event changes the reciprocal index by one, so a process connecting these even-separated indices has even order; no third-order term occurs for this single harmonic. The absent direct coefficient removes the first-order gap, not all possible virtual couplings. Exact symmetry protection would have to forbid the effective coupling at every order.

  • N. W. Ashcroft and N. D. Mermin, Solid State Physics (Holt, Rinehart and Winston, 1976), Chapter 9.
  • P. A. Lee, “Band Structure,” lecture notes for Theory of Solids I, MIT OpenCourseWare (2004), course materials.
  • S. H. Simon, The Oxford Solid State Basics (Oxford University Press, 2013), Chapter 15, Sec. 15.1.