International Conference
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Abstract We study the evolution of spins of binary black holes taking eccentricity into account. We are interested in determining the probability that these binaries may get locked in spin-orbit resonance configurations. We numerically evolve a large set of binaries starting from a large separation by using post-Newtonian approximation. The initial spin distribution is taken to be isotropic as is expected in many astrophysical environments. We find that a large fraction of the binaries get locked into or oscillate about the spin-orbit resonance configuration t owards the end of inspiral. This can be tested in future observations which, using our results, will allow us to deduce the initial spin distributions.
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