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- W2621092746 abstract "In this work we present an analytical gravitational self-force calculation of the spin-orbit precession along an eccentric orbit around a Schwarzschild black hole, following closely the recent prescription of Akcay, Dempsey, and Dolan, giving results to six post-Newtonian orders expanded in small eccentricity through ${e}^{2}$. We then transcribe this quantity within the effective-one-body (EOB) formalism, thereby determining several new, linear-in-mass-ratio contributions in the post-Newtonian expansion of the spin-orbit couplings entering the EOB Hamiltonian. Namely, we determine the second gyrogravitomagnetic ratio ${g}_{{S}_{*}}(r,{p}_{r},{p}_{ensuremath{phi}})$ up to order ${p}_{r}^{2}/{r}^{4}$ included." @default.
- W2621092746 created "2017-06-09" @default.
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- W2621092746 creator A5068982017 @default.
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- W2621092746 date "2017-09-11" @default.
- W2621092746 modified "2023-10-17" @default.
- W2621092746 title "Spin-orbit precession along eccentric orbits for extreme mass ratio black hole binaries and its effective-one-body transcription" @default.
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- W2621092746 doi "https://doi.org/10.1103/physrevd.96.064012" @default.
- W2621092746 hasPublicationYear "2017" @default.
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