Superfluidity in relativistic neutron stars

Simple item page
dc.creatorLanglois, David
dc.date2000-08-10
dc.date.accessioned2026-07-07T01:54:53Z
dc.date.available2026-07-07T01:54:53Z
dc.descriptionThe purpose of these notes is to give a brief review of superfluidity in neutron stars. After a short presentation explaining why and how superfluidity is expected in the crust and core of neutron stars, consequences on thermal evolution and rotational dynamics are discussed. The second part summarizes a formalism that has been recently developped to describe the hydrodynamics of superfluids or superconductors in the framework of general relativity. As an application, one can compute the oscillations of a two-component relativistic neutron star.
dc.descriptionInvited talk at the conference "Vortices in unconventional superconductors and superfluids" in Dresden (2000); 16 pages, 2 figures, LateX
dc.identifierhttps://arxiv.org/abs/astro-ph/0008161
dc.identifierhttp://arxiv.org/abs/astro-ph/0008161
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1466
dc.subjectAstrophysics
dc.subjectSuperconductivity
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSuperfluidity in relativistic neutron stars
dc.typetext

Files

Collections

arXiv