An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries [HEAP]

http://arxiv.org/abs/2110.09254


I present an analytical fit to the duration of the inspiral of two point masses driven by gravitational-wave emission. The fit is accurate to within 3% over the entire range of initial eccentricities from 0 to 0.99999.

Read this paper on arXiv…

I. Mandel
Tue, 19 Oct 21
4/98

Comments: N/A