Evolution of inspiral orbits around a Schwarzschild black hole
Niels WarburtonSchool of Mathematics, University of Southampton, Southampton SO17 1BJ, United KingdomSarp AkçaySchool of Mathematics, University of Southampton, Southampton SO17 1BJ, United KingdomLeor BarackSchool of Mathematics, University of Southampton, Southampton SO17 1BJ, United KingdomJ. R. GairInstitute of Astronomy, Madingley Road, Cambridge, CB3 0HA, United KingdomNorichika SagoYukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
2012en
ABI
Annotatsiya
We present results from calculations of the orbital evolution in eccentric binaries of nonrotating black holes with extreme mass ratios. Our inspiral model is based on the method of osculating geodesics, and is the first to incorporate the full gravitational self-force (GSF) effect, including conservative corrections. The GSF information is encapsulated in an analytic interpolation formula based on numerical GSF data for over a thousand sample geodesic orbits. We assess the importance of including conservative GSF corrections in waveform models for gravitational-wave searches.
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