Relations between three formalisms for irrotational binary neutron stars in general relativity

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dc.creatorGourgoulhon, Eric
dc.date1998-04-22
dc.date.accessioned2026-07-07T03:32:21Z
dc.date.available2026-07-07T03:32:21Z
dc.descriptionVarious formalisms proposed recently for irrotational binary systems in general relativity are compared and explicit relations between them are exhibited. It is notably shown that the formalisms of (i) Teukolsky, (ii) Shibata and (iii) Bonazzola et al. (as corrected by Asada) are equivalent, i.e. yield exactly the same solution, although the former two are simpler than the latter one.
dc.description5 pages, REVTeX, submitted as a brief report to Physical Review D
dc.identifierhttps://arxiv.org/abs/gr-qc/9804054
dc.identifierhttp://arxiv.org/abs/gr-qc/9804054
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36199
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleRelations between three formalisms for irrotational binary neutron stars in general relativity
dc.typetext

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