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arXiv · 2111.08033

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

Adrian S. Hamers
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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. 2021-11-15. An improved numerical fit to the peak harmonic gravitational wave frequency emitted by an eccentric binary. https://doi.org/10.3847/2515-5172%2Fac3d98

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