Deconfinement Phase Transition Heating and Thermal Evolution of Neutron Stars

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dc.creatorKang, Miao
dc.creatorPan, Nana
dc.creatorWang, Xiaodong
dc.date2007-11-03
dc.date2007-11-08
dc.date.accessioned2026-07-07T11:12:53Z
dc.date.available2026-07-07T11:12:53Z
dc.descriptionThe deconfinement phase transition will lead to the release of latent heat during spins down of neutron stars if the transition is the first-order one.We have investigated the thermal evolution of neutron stars undergoing such deconfinement phase transition. The results show that neutron stars may be heated to higher temperature.This feature could be particularly interesting for high temperature of low-magnetic field millisecond pulsar at late stage.
dc.description4 pages, to be published by American Institute of Physics, ed. D.Lai, X.D.Li and Y.F.Yuan, as the Proceedings of the conference Astrophysics of Compact Objects
dc.identifierhttps://arxiv.org/abs/0711.0443
dc.identifierhttp://arxiv.org/abs/0711.0443
dc.identifierAIPConf.Proc.968:203-205,2008
dc.identifierdoi:10.1063/1.2840397
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191530
dc.subjectAstrophysics
dc.titleDeconfinement Phase Transition Heating and Thermal Evolution of Neutron Stars
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