Coalescence of Binary Neutron Stars

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dc.creatorOohara, Ken-ichi
dc.creatorNamamura, Takashi
dc.date1996-06-29
dc.date.accessioned2026-07-07T02:21:26Z
dc.date.available2026-07-07T02:21:26Z
dc.descriptionThe most important sources for laser-interferometric gravitational-wave detectors like LIGO or VIRGO are catastrophic events such as coalescence of a neutron-star binary. The final phase, or the last three milliseconds, of coalescence is considered. We describe results of numerical simulations of coalescing binary neutron stars using Newtonian and post-Newtonian hydrodynamics code and then discuss recent development of our 3D GR code.
dc.description30 pages, LaTeX, 17 PostScript figures, Lecture delivered at Les Houches School ``Astrophysical Sources of Gravitational Radiation'' (Les Houches, France, Sept. 26 - Oct. 6, 1995). To be published in the Proceedings (eds. J.-A. Marck and J.-P. Lasota)
dc.identifierhttps://arxiv.org/abs/astro-ph/9606179
dc.identifierhttp://arxiv.org/abs/astro-ph/9606179
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10544
dc.subjectAstrophysics
dc.titleCoalescence of Binary Neutron Stars
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