On Estimation of the Post-Newtonian Parameters in the Gravitational-Wave Emission of a Coalescing Binary

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dc.creatorKrólak, Andrzej
dc.creatorKokkotas, Kostas D.
dc.creatorSchäfer, Gerhard
dc.date1995-03-07
dc.date.accessioned2026-07-07T11:46:22Z
dc.date.available2026-07-07T11:46:22Z
dc.descriptionThe effect of the recently obtained 2nd post-Newtonian corrections on the accuracy of estimation of parameters of the gravitational-wave signal from a coalescing binary is investigated. It is shown that addition of this correction degrades considerably the accuracy of determination of individual masses of the members of the binary. However the chirp mass and the time parameter in the signal is still determined to a very good accuracy. The possibility of estimation of effects of other theories of gravity is investigated. The performance of the Newtonian filter is investigated and it is compared with performance of post-Newtonian search templates introduced recently. It is shown that both search templates can extract accurately useful information about the binary.
dc.description34 pages, 118Kb, LATEX format, submitted to Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/gr-qc/9503013
dc.identifierhttp://arxiv.org/abs/gr-qc/9503013
dc.identifierPhys.Rev.D52:2089-2111,1995
dc.identifierdoi:10.1103/PhysRevD.52.2089
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202204
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn Estimation of the Post-Newtonian Parameters in the Gravitational-Wave Emission of a Coalescing Binary
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