An improved numerical fit to the peak harmonic gravitational wave frequency emitted by an eccentric binary

Published 15 Nov 2021 in gr-qc and astro-ph.HE | (2111.08033v2)

Abstract: I present a numerical fit to the peak harmonic gravitational wave frequency emitted by an eccentric binary system in the post-Newtonian approximation. This fit significantly improves upon a previous commonly-used fit in population synthesis studies, in particular for eccentricities $\lesssim 0.8$.

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Adrian S. Hamers

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