Self-energy Effects in the Superfluidity of Neutron Matter

Abstract

The superfluidity of neutron matter in the channel ${}^1{S}_0$ is studied by taking into account the effect of the ground-state correlations in the self-energy. To this purpose the gap equation has been solved within the generalized Gorkov approach. A sizeable suppression of the energy gap is driven by the quasi-particle strength around the Fermi surface.

arXiv comment8 pages and 3 figures

References in corpus (4)

• Effective density dependent pairing forces in the T=1 and T=0 channels
• Superfluid nuclear matter calculations
• Dispersive effects in neutron matter superfluidity
• Frictional Heating and Neutron Star Thermal Evolution

Cited by in corpus (30)

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