Setting Vq = VLq = ∆(0) q /(ℏkF q), along with ∆q = ∆(0) q , in Eqs

Superfluid phase: onset of gapless regime Vq = VLq The specific heat is amenable to an analytical approximation when the effective superfluid velocity is equal to Landau’s critical

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it

browse 1 citing papers

representative citing papers

Gapless superfluidity in neutron stars: Thermal properties

nucl-th · 2024-03-12 · unverdicted · novelty 6.0

Nuclear EDF theory predicts gapless superfluidity in neutron stars with unsuppressed specific heat at low temperatures.

citing papers explorer

Showing 1 of 1 citing paper.

Gapless superfluidity in neutron stars: Thermal properties nucl-th · 2024-03-12 · unverdicted · none · ref 5
Nuclear EDF theory predicts gapless superfluidity in neutron stars with unsuppressed specific heat at low temperatures.

Setting Vq = VLq = ∆(0) q /(ℏkF q), along with ∆q = ∆(0) q , in Eqs

fields

years

verdicts

representative citing papers

citing papers explorer