Quasiequilibrium sequences of binary strange quark stars in general relativity

Simple item page
dc.creatorLimousin, Francois
dc.creatorGondek-Rosinska, Dorota
dc.creatorGourgoulhon, Eric
dc.date2004-11-30
dc.date.accessioned2026-07-07T03:29:13Z
dc.date.available2026-07-07T03:29:13Z
dc.descriptionInspiraling compact binaries are expected to be the strongest sources of gravitational waves for VIRGO, LIGO and other laser interferometers. We present the first computations of quasi-equilibrium sequences of compact binaries containing two strange quark stars (which are currently considered as a possible alternative to neutron stars). We study a precoalescing stage in the conformal flatness approximation of general relativity using a multidomain spectral method. A hydrodynamical treatment is performed under the assumption that the flow is irrotational.
dc.description4 pages, 2 PostScript figures, to appear in the Proceedings of the SF2A 04, Paris, France
dc.identifierhttps://arxiv.org/abs/gr-qc/0411147
dc.identifierhttp://arxiv.org/abs/gr-qc/0411147
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35128
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuasiequilibrium sequences of binary strange quark stars in general relativity
dc.typetext

Files

Collections

arXiv