Nuclear Superfluidity and Cooling Time of Neutron-Star Crust

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dc.creatorMonrozeau, C.
dc.creatorMargueron, J.
dc.creatorSandulescu, N.
dc.date2007-03-21
dc.date.accessioned2026-07-07T10:38:41Z
dc.date.available2026-07-07T10:38:41Z
dc.descriptionWe analyse the effect of neutron superfluidity on the cooling time of inner crust matter in neutron stars, in the case of a rapid cooling of the core. The specific heat of the inner crust, which determines the thermal response of the crust, is calculated in the framework of HFB approach at finite temperature. The calculations are performed with two paring forces chosen to simulate the pairing properties of uniform neutron matter corresponding respectively to Gogny-BCS approximation and to many-body techniques including polarisation effects. Using a simple model for the heat transport across the inner crust, it is shown that the two pairing forces give very different values for the cooling time.
dc.description6 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0703064
dc.identifierhttp://arxiv.org/abs/nucl-th/0703064
dc.identifierPhys.Rev.C75:065807,2007
dc.identifierdoi:10.1103/PhysRevC.75.065807
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180809
dc.subjectNuclear Theory
dc.titleNuclear Superfluidity and Cooling Time of Neutron-Star Crust
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