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arXiv · 1506.04768

Spin flips in generic black hole binaries

Carlos O. Lousto·James Healy·Hiroyuki Nakano
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Abstract

We study the spin dynamics of individual black holes in a binary system. In particular we focus on the polar precession of spins and the possibility of a complete flip of spins with respect to the orbital plane. We perform a full numerical simulation that displays these characteristics. We evolve equal mass binary spinning black holes for $t=20,000M$ from an initial proper separation of $d=25M$ down to merger after 48.5 orbits. We compute the gravitational radiation from this system and compare it to 3.5 post-Newtonian generated waveforms finding close agreement. We then further use 3.5 post-Newtonian evolutions to show the extension of this spin {flip-flop} phenomenon to unequal mass binaries. We also provide analytic expressions to approximate the maximum {flip-flop} angle and frequency in terms of the binary spins and mass ratio parameters at a given orbital radius. Finally we discuss the effect this spin {flip-flop} would have on accreting matter and other potential observational effects.

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BibTeXRIS

Carlos O. Lousto, James Healy, Hiroyuki Nakano. 2015-06-15. Spin flips in generic black hole binaries. https://doi.org/10.1103/physrevd.93.044031

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