Math 2.0

Statistical mechanics, structure of matter Definition

BCS theory

Builds on Fermi surfaceFermi–Dirac statistics

Definition

Consider spin-1/21/2 electrons with creation and annihilation operators ckσ†,ckσc^\dagger_{k\sigma}, c_{k\sigma} for momentum kk and spin σ∈{↑,↓}\sigma \in \set{\uparrow, \downarrow}, single-particle energies εk\varepsilon_k, chemical potential μ\mu and ξk=εk−μ\xi_k = \varepsilon_k - \mu. The reduced BCS Hamiltonian is H=∑k,σξk ckσ†ckσ−∑k,k′Vkk′ ck↑†c−k↓†c−k′↓ck′↑,H = \sum_{k,\sigma} \xi_k \, c^\dagger_{k\sigma} c_{k\sigma} - \sum_{k, k'} V_{kk'} \, c^\dagger_{k\uparrow} c^\dagger_{-k\downarrow} c_{-k'\downarrow} c_{k'\uparrow}, where, in the BCS model, Vkk′=V>0V_{kk'} = V > 0 if ∣ξk∣≤ℏωD\abs{\xi_k} \le \hbar\omega_D and ∣ξk′∣≤ℏωD\abs{\xi_{k'}} \le \hbar\omega_D, and Vkk′=0V_{kk'} = 0 otherwise, for a cutoff energy ℏωD\hbar\omega_D. The BCS state is ∣Ψ⟩=∏k(uk+vk ck↑†c−k↓†)∣0⟩,∣uk∣2+∣vk∣2=1.\lvert \Psi \rangle = \prod_k \big(u_k + v_k \, c^\dagger_{k\uparrow} c^\dagger_{-k\downarrow}\big) \lvert 0 \rangle, \qquad \abs{u_k}^2 + \abs{v_k}^2 = 1. Minimising the energy over such states at zero temperature gives the gap equation Δk=∑k′Vkk′Δk′2Ek′,Ek=ξk2+∣Δk∣2,\Delta_k = \sum_{k'} V_{kk'} \frac{\Delta_{k'}}{2E_{k'}}, \qquad E_k = \sqrt{\xi_k^2 + \abs{\Delta_k}^2}, where EkE_k is the energy of a quasiparticle excitation.

Remarks

In the BCS model Δk=Δ\Delta_k = \Delta is constant in the shell ∣ξk∣≤ℏωD\abs{\xi_k} \le \hbar\omega_D. Replacing the sum by an integral with density of states N(0)N(0) per spin at the Fermi surface, a nonzero solution satisfies 1=N(0)V∫0ℏωDdξ/ξ2+Δ21 = N(0)V \int_0^{\hbar\omega_D} d\xi / \sqrt{\xi^2 + \Delta^2}. So Δ=ℏωD/sinh⁡(1/(N(0)V))\Delta = \hbar\omega_D / \sinh\big(1/(N(0)V)\big), which is close to 2ℏωDe−1/(N(0)V)2\hbar\omega_D e^{-1/(N(0)V)} for weak coupling. At temperature T>0T > 0 the factor 1/(2Ek)1/(2E_k) becomes tanh⁡(Ek/2kBT)/(2Ek)\tanh(E_k / 2k_B T)/(2E_k), and Δ\Delta vanishes at TcT_c with kBTc≈1.13 ℏωDe−1/(N(0)V)k_B T_c \approx 1.13\, \hbar\omega_D e^{-1/(N(0)V)}.

Example: Δ=0\Delta = 0 always solves the gap equation; it is the normal state, a filled Fermi sea with vk=1v_k = 1 for ξk<0\xi_k < 0 and vk=0v_k = 0 for ξk>0\xi_k > 0. For V>0V > 0 the nonzero solution has lower energy, however small VV is.

Non-example: for a repulsive interaction, V<0V < 0, the right side of 1=N(0)V∫dξ/ξ2+Δ21 = N(0)V \int d\xi / \sqrt{\xi^2 + \Delta^2} is negative, so the only solution is Δ=0\Delta = 0 and there is no superconductivity.

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Further reading

  1. Web https://en.wikipedia.org/wiki/BCS_theory
About this page
Tag3ECCH466Q0
URIm2://3ECCH466Q0
Kinddefinition
WritingW0 stub
MSC82D55, 81V74
DefinesBCS theory
UsesFermi surface, Fermi–Dirac statistics
Changed3 November 2026

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