Gravitational Waves from Phase Transition of Accreting Neutron Stars

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dc.creatorCheng, K. S.
dc.creatorDai, Z. G.
dc.date1997-04-16
dc.date.accessioned2026-07-07T11:46:07Z
dc.date.available2026-07-07T11:46:07Z
dc.descriptionWe propose that when neutron stars in low-mass X-ray binaries accrete sufficient mass and become millisecond pulsars, the interiors of these stars may undergo phase transitions, which excite stellar radial oscillations. We show that the radial oscillations will be mainly damped by gravitational-wave radiation instead of internal viscosity. The gravitational waves can be detected by the advanced Laser Interferometer Gravitational-Wave Observatory at a rate of about three events per year.
dc.descriptionLatex, article style, approximately 10 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9704161
dc.identifierhttp://arxiv.org/abs/astro-ph/9704161
dc.identifierAstrophys.J.492:281-285,1998
dc.identifierdoi:10.1086/305040
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202115
dc.subjectAstrophysics
dc.titleGravitational Waves from Phase Transition of Accreting Neutron Stars
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