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Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order

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arxiv gr-qc/9602024 v1 pith:2TZY23UO submitted 1996-02-13 gr-qc

Luc Blanchet , Bala R. Iyer , Clifford M. Will , Alan G. Wiseman This is my paper · ORCID
classification gr-qc
keywords gravitationalwaveformsbinariescompactfieldinspirallingsecond-post-newtoniananalysis
verification ladder T0 review T1 audit T2 compute T3 formal
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The two independent ``plus" and ``cross" polarization waveforms associated with the gravitational waves emitted by inspiralling, non-spinning, compact binaries are presented, ready for use in the data analysis of signals received by future laser interferometer gravitational-wave detectors such as LIGO and VIRGO. The computation is based on a recently derived expression of the gravitational field at the second-post-Newtonian approximation of general relativity beyond the dominant (Newtonian) quadrupolar field. The use of these theoretical waveforms to make measurements of astrophysical parameters and to test the nature of relativistic gravity is discussed.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM

    gr-qc 2024-12 conditional novelty 7.0 of 10

    The authors obtain, for the first time, 3PN-accurate eccentric-orbit fluxes, radiation-reaction force, and waveform modes in the effective-one-body formalism, and use them to build the SEOBNRv5EHM inspiral model.

  2. The Chirp-Mass Ladder: A New Rung Emerges

    astro-ph.HE 2026-06 unverdicted novelty 5.5 of 10

    The chirp-mass distribution of GW-detected binary black holes shows a ladder of peaks doubling in mass, with a new intermediate peak at 19 solar masses confirming a prior prediction from the hierarchical merger model.

  3. Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries

    gr-qc 2024-06 conditional novelty 4.0 of 10

    4.5PN and 2SF calculations of gravitational energy flux for quasicircular compact binaries agree.

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