Implication of Existence of Hybrid stars and Theoretical Expectation of Submillisecond Pulsars

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dc.creatorZheng, Xiaoping
dc.creatorPan, Nana
dc.creatorYang, Shuhua
dc.creatorLiu, Xuewen
dc.creatorKang, Miao
dc.creatorLi, Jiarong
dc.date2006-09-01
dc.date2008-01-08
dc.date.accessioned2026-07-07T10:23:32Z
dc.date.available2026-07-07T10:23:32Z
dc.descriptionWe derive the bulk viscous damping timescale of hybrid stars, neutron stars with quark matter core. The r-mode instability windows of the stars show that the theoretical results are consistent with the rapid rotation pulsar data, which may give an indication for the existence of quark matter in the interior of neutron stars. Hybrid stars instead of neutron or strange stars may lead to submillisecond pulsars.
dc.description9 pages,3 figures, accepted by New Astronomy
dc.identifierhttps://arxiv.org/abs/astro-ph/0609011
dc.identifierhttp://arxiv.org/abs/astro-ph/0609011
dc.identifierNewAstron.12:165-168,2006
dc.identifierdoi:10.1016/j.newast.2006.08.002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175864
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleImplication of Existence of Hybrid stars and Theoretical Expectation of Submillisecond Pulsars
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