Thermal Evolution of Strange Stars

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Dec 2007Embargo end date: 01 Jan 2007Publisher:IOP PublishingJournal:Publications of the Astronomical Society of the Pacific, volume 119, pages 1,367-1,370 (issn: 0004-6280, eissn: 1538-3873,

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Authors: Xia, Zhou; Lingzhi, Wang; Aizhi, Zhou;

doi: 10.1086/524711 , 10.48550/arxiv.0709.0214

arXiv: 0709.0214

Thermal Evolution of Strange Stars

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Abstract

We 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.

13 pages, 2 figures

Related Organizations

Central China Normal University
China (People's Republic of)

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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NEANIAS Space Research Community