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- W3182876307 abstract "Within the framework of self-force theory, we compute the gravitational-wave energy flux through second order in the mass ratio for compact binaries in quasicircular orbits. Our results are consistent with post-Newtonian calculations in the weak field, and they agree remarkably well with numerical-relativity simulations of comparable-mass binaries in the strong field. We also find good agreement for binaries with a spinning secondary or a slowly spinning primary. Our results are key for accurately modeling extreme-mass-ratio inspirals and will be useful in modeling intermediate-mass-ratio systems." @default.
- W3182876307 created "2021-07-19" @default.
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- W3182876307 date "2021-10-08" @default.
- W3182876307 modified "2023-10-14" @default.
- W3182876307 title "Gravitational-Wave Energy Flux for Compact Binaries through Second Order in the Mass Ratio" @default.
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- W3182876307 doi "https://doi.org/10.1103/physrevlett.127.151102" @default.
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