Cooper Pair
How Paired Electrons Enable Lossless Supercurrent
In a normal metal, conduction electrons scatter off lattice defects and thermal vibrations, dissipating energy as heat and producing ordinary resistance. Below the critical temperature, a fundamentally different mechanism takes over. Leon Cooper demonstrated in 1956 that the Fermi sea is unstable against an arbitrarily weak attractive interaction, and that two electrons near the Fermi surface will bind into a pair with lower total energy. The attraction is not direct; it is mediated by the lattice. One electron polarizes the positively charged ion cores as it passes, and a second electron with opposite momentum is drawn into the trailing region of enhanced positive charge. Because the ions respond on the slow timescale of the Debye frequency, the two electrons need not be close in space, which is the origin of the very large pair size.
The full many-body extension by Bardeen, Cooper, and Schrieffer (BCS) showed that all such pairs condense into one macroscopic wavefunction with a common phase. This condensate is separated from single-particle excitations by the superconducting energy gap, 2Δ, which at zero temperature equals about 3.52 kBTc for a conventional weak-coupling superconductor. For niobium, the workhorse material of superconducting RF cavities, Tc ≈ 9.2 K gives a gap of roughly 2.8 meV. Because no low-energy states exist within the gap, the pairs cannot scatter individually, and a DC supercurrent flows indefinitely without loss.
At microwave frequencies the picture is more subtle. The oscillating field repeatedly accelerates the inertial pair condensate, and the resulting kinetic inductance means screening is imperfect. A residual field reaches the thermally excited quasiparticles, producing a small but nonzero surface resistance described by the Mattis-Bardeen theory. This is why a 1.3 GHz niobium accelerator cavity is operated near 2 K to suppress quasiparticles and reach surface resistance on the order of 10 nΩ, far below the few mΩ of copper at the same frequency.
Governing Relations for Cooper Pairing
2Δ(0) ≈ 3.52 × kBTc
Pippard / BCS Coherence Length:
ξ0 = (ℏ × vF) / (π × Δ)
Mattis-Bardeen RF Surface Resistance:
Rs ≈ A × (ω² / T) × exp(−Δ / kBT) + Rres
Where kB = Boltzmann constant, Tc = critical temperature, ℏ = reduced Planck constant, vF = Fermi velocity, Δ = half the energy gap, ω = angular frequency, Rres = residual resistance floor. Example (niobium): Tc ≈ 9.2 K → 2Δ(0) ≈ 2.8 meV, ξ0 ≈ 38 nm.
Superconductor Pairing Parameters
| Material | Tc (K) | Gap 2Δ(0) (meV) | Coherence Length ξ0 | RF Use Case |
|---|---|---|---|---|
| Aluminum | 1.2 | 0.36 | ≈ 1600 nm | Qubits, kinetic-inductance detectors |
| Niobium | 9.2 | 2.8 | ≈ 38 nm | SRF accelerator cavities |
| NbTiN | 15 to 16 | ~4.5 | ≈ 4 to 5 nm | High-kinetic-inductance resonators |
| Nb₃Sn | 18 | ~6.5 | ≈ 3 nm | Higher-temperature SRF coatings |
| YBCO (high-Tc) | 92 | ~30 to 40 | ≈ 1.5 nm (ab-plane) | Cryo-cooled microwave filters |
Frequently Asked Questions
Why do two electrons attract each other to form a Cooper pair?
Two electrons repel via Coulomb force, but in a metal below Tc a phonon-mediated attraction wins out near the Fermi surface. A moving electron distorts the positive ion lattice, and a second electron of opposite momentum and spin is drawn toward that transient positive charge. Cooper showed in 1956 that even a weak attraction binds the pair into a lower-energy spin-singlet state with zero net momentum, with the Debye energy setting the attraction scale.
How large is a Cooper pair compared to the electron spacing?
The pair size is set by the coherence length, ξ0 = ℏvF / (πΔ): about 38 nm in niobium and roughly 1600 nm in aluminum. Since conduction electrons sit only ~0.2 to 0.3 nm apart, one pair overlaps the centers of millions of others. That overlap forces all pairs into a single coherent quantum state with one phase, which produces flux quantization, the Josephson effect, and lossless RF screening currents.
Why is RF surface resistance not exactly zero even though Cooper pairs carry no DC loss?
At microwave frequencies the AC field keeps accelerating the inertial pair condensate, so its kinetic inductance prevents perfect screening. A residual field then acts on thermally excited quasiparticles, dissipating power. The Mattis-Bardeen result gives Rs ∝ (ω²/T) exp(−Δ/kBT) plus a residual floor, so a 1.3 GHz niobium cavity cooled to 2 K reaches ~10 nΩ but never a true zero.