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Superfluid phase: gapless regime VLq < Vq ≤ V(0) cq For effective superfluid velocities larger than VLq, ∆ q no longer remains constant but decreases with increasing Vq, vanishe

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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.

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Gapless superfluidity in neutron stars: Thermal properties nucl-th · 2024-03-12 · unverdicted · none · ref 6
Nuclear EDF theory predicts gapless superfluidity in neutron stars with unsuppressed specific heat at low temperatures.

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