Gravitational-Wave Energy Flux for Compact Binaries through Second Order in the Mass Ratio
Within the framework of self-force theory, we compute the gravitational-wave energy flux through second order in the mass ratio for compact binaries in quasicircular orbits. Our results are consistent with post-Newtonian calculations in the weak field, and they agree remarkably well with numerical-r...
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Veröffentlicht in: | Physical review letters 2021-10, Vol.127 (15), p.1-151102, Article 151102 |
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creator | Warburton, Niels Pound, Adam Wardell, Barry Miller, Jeremy Durkan, Leanne |
description | Within the framework of self-force theory, we compute the gravitational-wave energy flux through second order in the mass ratio for compact binaries in quasicircular orbits. Our results are consistent with post-Newtonian calculations in the weak field, and they agree remarkably well with numerical-relativity simulations of comparable-mass binaries in the strong field. We also find good agreement for binaries with a spinning secondary or a slowly spinning primary. Our results are key for accurately modeling extreme-mass-ratio inspirals and will be useful in modeling intermediate-mass-ratio systems. |
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subjects | Gravitational waves Relativity Wave power |
title | Gravitational-Wave Energy Flux for Compact Binaries through Second Order in the Mass Ratio |
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