Darwin-Riemann problems in general relativity

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dc.creatorBonazzola, S.
dc.creatorGourgoulhon, E.
dc.creatorGrandclement, P.
dc.creatorMarck, J. -A.
dc.date1999-09-06
dc.date.accessioned2026-07-07T11:08:47Z
dc.date.available2026-07-07T11:08:47Z
dc.descriptionA review is given of recent results about the computation of irrotational Darwin-Riemann configurations in general relativity. Such configurations are expected to represent fairly well the late stages of inspiralling binary neutron stars.
dc.description20 pages, 11 PostScript figures, uses PTPTeX, to appear in the Proceedings of Yukawa International Seminar 99 "Black Holes and Gravitational Waves", edited by T. Nakamura & H. Kodama, Prog. Theor. Phys. Suppl
dc.identifierhttps://arxiv.org/abs/gr-qc/9909020
dc.identifierhttp://arxiv.org/abs/gr-qc/9909020
dc.identifierProg.Theor.Phys.Suppl.136:216,1999
dc.identifierdoi:10.1143/PTPS.136.216
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190256
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDarwin-Riemann problems in general relativity
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