Detection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations

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dc.creatorSintes, A. M.
dc.creatorVecchio, A.
dc.date2000-05-16
dc.date.accessioned2026-07-07T03:24:56Z
dc.date.available2026-07-07T03:24:56Z
dc.descriptionThe set up of matched filters for the detection of gravitational waves from in-spiraling compact binaries is usually carried out using the restricted post-Newtonian approximation: the filter phase is modelled including post-Newtonian corrections, whereas the amplitude is retained at the Newtonian order. Here we investigate the effects of the introduction of post-Newtonian corrections also to the amplitude and we discuss some of the implications for signal detection and parameter estimation.
dc.descriptionLatex, 6 pages. To appear in: "Rencontres de Moriond: Gravitational waves and experimetal gravity". Edt. J. Dumarchez; Editions Frontieres, France
dc.identifierhttps://arxiv.org/abs/gr-qc/0005058
dc.identifierhttp://arxiv.org/abs/gr-qc/0005058
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33532
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDetection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations
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