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Gravitational-wave equation in effective one-body background for spinless binary

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arxiv 2301.08318 v1 pith:KEPJNGNB submitted 2023-01-18 gr-qc astro-ph.HE

classification gr-qcastro-ph.HE
keywords backgroundbinaryeffectiveequationgravitational-waveone-bodyspinlessavailable
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We construct the gravitational-wave equation in the background of the effective one-body system for the spinless binary, which is in general available with the spherically symmetric background as well. The gauge conditions are given in terms of the metric perturbation.

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  1. Teukolsky-like equations with various spins in a deformed Kerr spacetime

    gr-qc 2024-12 conditional novelty 6.0 of 10

    On a Kerr spacetime with an arbitrary radial deformation L(r), all massless spin fields satisfy one unified Teukolsky-like master equation that separates into a standard angular part and a deformed radial part.

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