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• W2022766564 abstract "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 $1/8ensuremath{le}{m}_{1}/{m}_{2}ensuremath{le}1$ 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 ${m}_{1}/{m}_{2}ensuremath{rightarrow}{m}_{1}{m}_{2}/({m}_{1}+{m}_{2}{)}^{2}$]. Our results can inform a universal analytic model of the two-body dynamics, crucial for ongoing and future gravitational-wave searches." @default.
• W2022766564 created "2016-06-24" @default.
• W2022766564 creator A5004437377 @default.
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• W2022766564 date "2011-09-30" @default.
• W2022766564 modified "2023-10-15" @default.
• W2022766564 title "Periastron Advance in Black-Hole Binaries" @default.
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• W2022766564 doi "https://doi.org/10.1103/physrevlett.107.141101" @default.
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