BCS coherence factors Created 2026-10-06 Updated 2026-10-18
For real gap and the particle-hole block , the BCS coherence factors obey , and , where . They diagonalize the Bogoliubov--de Gennes Hamiltonian and give the empty/pair amplitudes of the BCS ground state. Their relative sign depends on the pairing convention.
For an original check, write with constant real . At , the BCS coherence factors give . At , they give ; at these values exchange places. Thus the zero-temperature occupation rounds the normal Fermi sea's step over an energy interval of order . This mixing is strongest at the Fermi surface, where the BCS quasiparticle spectrum has its minimum.
BCS quasiparticle spectrum 2026-10-18
The BCS quasiparticle spectrum is the positive excitation energy obtained by diagonalizing the paired particle-hole block. Here the weak coupling shell model has : the minimum lies inside the pairing shell, and states outside it cost more. To derive it for a uniform isotropic real , measure the normal-state energy from the chemical potential, , and use the same sign convention as the BCS coherence factors:Its eigenvalues are , where . The positive is the cost of creating a quasiparticle above the BCS ground state. The lower branch is its particle-hole partner in this doubled matrix description, not an excitation that lowers the ground state energy without bound.
The location and value of the minimum follow directly:The unique minimum as a function of is , at the normal-state Fermi surface. On an isotropic three-dimensional Fermi surface it occurs for every direction of , rather than at a unique point of momentum space. Near that minimum,Farther away, when . For the illustrative example, a state at costs rather than the minimum .
Put and . The BCS quasiparticle spectrum has , so on either inverse branchConservation of states on one branch gives . Consequently the single-branch expression requested in the source isThere are no such states for in this ideal fully gapped model. Near the edge the density of states diverges as , an integrable singularity; at large it approaches its normal-state value.
Counting qualification. The energy map in the source is two-to-one. If literally counts all normal-state levels both above and below , the unweighted positive-energy quasiparticle density from a folded spectrum must sum both preimages, and is insteadAlready at , folding into doubles the positive-axis density. Thus the printed formula is not the unweighted count of all states under the literal mapping without an additional normalization convention.
There is also a standard physical quantity with exactly the printed normalization: the BCS electronic density of states, measured for example by single-electron superconducting tunneling. At positive , the electron spectral weights of the two roots are the BCS coherence factors . They sum to one, so the weighted sum is . This supplies a valid electronic-DOS interpretation, while keeping it distinct from counting every positive-energy excitation. Spin degeneracy must be included consistently in and the transformed density; it does not remove the branch-counting issue.
Superconducting energy gap 2026-10-18
In this fully gapped isotropic BCS quasiparticle spectrum, is the minimum single-quasiparticle excitation energy. The interval between and has width . A process that creates two quasiparticles from the BCS ground state has an energetic threshold , subject also to its transition-selection rules.[ref]
Microscopic Quantum Interference Effects in the Theory of Superconductivity by Leon Neil Cooper. 1972 lecture, excitation spectrum and correlated background, pp.78–80
For example, two independently created excitations with cost . With the chosen cutoff example this is , while adding one excitation costs at least . This factor of two matters when comparing photon absorption with the Giaever superconducting tunnelling experiment. Quantum tunnelling from a normal metal can add one excitation to a sample exhibiting superconductivity; with two gapped electrodes, their excitation costs add. A minimum excitation cost is an energetic condition; the measured onset can additionally depend on temperature and on the available transitions.
