New Class of Gravitational Wave Templates for Inspiralling Compact Binaries

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dc.creatorGopakumar, Achamveedu
dc.date2007-12-19
dc.date.accessioned2026-07-07T08:50:23Z
dc.date.available2026-07-07T08:50:23Z
dc.descriptionCompact binaries inspiralling along quasi-circular orbits are the most plausible gravitational wave (GW) sources for the operational, planned and proposed laser interferometers. We provide new class of restricted post-Newtonian accurate GW templates for non-spinning compact binaries inspiralling along PN accurate quasi-circular orbits. Arguments based on data analysis, theoretical and astrophysical considerations are invoked to show why these time-domain Taylor approximants should be interesting to various GW data analysis communities.
dc.description5 pages
dc.identifierhttps://arxiv.org/abs/0712.3236
dc.identifierhttp://arxiv.org/abs/0712.3236
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/144589
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNew Class of Gravitational Wave Templates for Inspiralling Compact Binaries
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