Thermal Evolution of Isolated Neutron Stars. II

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dc.creatorPage, Dany
dc.date1998-02-13
dc.date.accessioned2026-07-07T02:26:04Z
dc.date.available2026-07-07T02:26:04Z
dc.descriptionAfter a brief summary of neutron star cooling theory I present results which emphasize the importance of baryon pairing in the neutron star core. I show how the thermal evolution may be totally controlled by pairing for models which include only nucleons and models containing also hyperons. Finally, I consider the thermal evolution of ultramagnetized neutron stars whose existence has been inferred from the soft gamma repeaters.
dc.description8 pages LaTeX with 3 eps figures. Uses neu.sty and tron,sty (included). Invited talk at the meeting `Neutron Stars and Pulsars', Tokyo, Nov. 1997
dc.identifierhttps://arxiv.org/abs/astro-ph/9802171
dc.identifierhttp://arxiv.org/abs/astro-ph/9802171
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12128
dc.subjectAstrophysics
dc.titleThermal Evolution of Isolated Neutron Stars. II
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