Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms

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dc.creatorPoisson, Eric
dc.date1998-01-12
dc.date.accessioned2026-07-07T03:32:09Z
dc.date.available2026-07-07T03:32:09Z
dc.descriptionThe accuracy of the post-Newtonian waveforms, both in standard and Pade form, is determined by computing their matched-filtering overlap integral with a reference waveform obtained from black-hole perturbation theory.
dc.description3 pages, ReVTeX, to appear in the Proceedings of the Second Gravitational Wave Data Analysis Workshop, held in Orsay, France
dc.identifierhttps://arxiv.org/abs/gr-qc/9801038
dc.identifierhttp://arxiv.org/abs/gr-qc/9801038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36126
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms
dc.typetext

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