Quark matter imprint on Gravitational Waves from oscillating stars

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dc.creatorBenhar, Omar
dc.creatorFerrari, Valeria
dc.creatorGualtieri, Leonardo
dc.creatorMarassi, Stefania
dc.date2006-03-17
dc.date2007-04-02
dc.date.accessioned2026-07-07T11:03:58Z
dc.date.available2026-07-07T11:03:58Z
dc.descriptionWe discuss the possibility that the detection of gravitational waves emitted by compact stars may allow to constrain the MIT bag model of quark matter equation of state. Our results show that the combined knowledge of the frequency of the emitted gravitational wave and of the mass, or the radiation radius, of the source allows one to discriminate between strange stars and neutron stars and set stringent bounds on the bag constants.
dc.descriptionEight pages, four figures. Revised version, to appear on General Relativity and Gravitation
dc.identifierhttps://arxiv.org/abs/astro-ph/0603464
dc.identifierhttp://arxiv.org/abs/astro-ph/0603464
dc.identifierGen.Rel.Grav.39:1323,2007
dc.identifierdoi:10.1007/s10714-007-0444-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188733
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuark matter imprint on Gravitational Waves from oscillating stars
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