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2011

Periastron Advance in Black-Hole Binaries

Tiec, Alexandre Le, Mroué, Abdul H., Barack, Leor et al.

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The general relativistic (Mercury-type) periastron advance is calculated here for the first time with exquisite precision in full general relativity.

We use accurate numerical relativity simulations of spinless black hole binaries with mass ratios 1/8 < m1/m2 < 1 and compare with the predictions of several analytic approximation schemes.
We find the effective-one-body model to be remarkably accurate, and, surprisingly, so also the predictions of self-force theory [replacing m1/m2 --> m1m2/(m1+m2)^2].
Our results can inform a universal analytic model of the two-body dynamics, crucial for ongoing and future gravitational-wave searches.

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