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Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity · Around

2017

Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

Healy, James, Lousto, Carlos O., Nakano, Hiroyuki et al.

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We use post-Newtonian (PN) approximations to determine the initial orbital and spin parameters of black hole binaries that lead to low-eccentricity inspirals when evolved with numerical relativity techniques.

In particular, we seek initial configurations that lead to very small eccentricities at small separations, as is expected for astrophysical systems.
We consider three cases: (i) quasicircular orbits with no radial velocity, (ii) quasicircular orbits with an initial radial velocity determined by radiation reaction, and (iii) parameters obtained form evolution of the PN equations of motion from much larger separations.
We study seven cases of spinning, nonprecessing, unequal mass binaries.

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