Periastron Advance in Black-Hole Binaries
  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. 
Alexandre Le Tiec, Abdul H. Mrou\'e, Leor Barack, Alessandra Buonanno,   Harald P. Pfeiffer, Norichika Sago, Andrea Taracchini
gr-qc astro-ph.HE