Thermal Evolution of Strange Stars

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dc.creatorXia, Zhou
dc.creatorLingzhi, Wang
dc.creatorAizhi, Zhou
dc.date2007-09-03
dc.date.accessioned2026-07-07T08:54:43Z
dc.date.available2026-07-07T08:54:43Z
dc.descriptionWe investigated the thermal evolution of rotating strange stars with the deconfinement heating due to magnetic braking. We consider the stars consisting of either normal quark matter or color-flavor-locked phase. Combining deconfinement heating with magnetic field decay, we find that the thermal evolution curves are identical to pulsar data.
dc.description13 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/0709.0214
dc.identifierhttp://arxiv.org/abs/0709.0214
dc.identifierPASP, 119:1367-1370, 2007 December
dc.identifierdoi:10.1086/524711
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/146040
dc.subjectAstrophysics
dc.titleThermal Evolution of Strange Stars
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