Papers › An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries
An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries
Ilya Mandel
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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.
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