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- W2045142020 abstract "The effect of gravitational radiation reaction on circular orbits around a spinning (Kerr) black hole is computed to leading order in S (the magnitude of the spin angular momentum of the hole) and in the strength of gravity M/r (where M is the mass of the black hole, r is the orbital radius, and G=c=1). The radiation reaction makes the orbit shrink but leaves it circular and drives the orbital plane very slowly toward antialignment with the spin of the hole: tan(ensuremath{iota}/2)=tan(${mathrm{ensuremath{iota}}}_{0}$/2)[1+(61/72)(S/${mathit{M}}^{2}$)(M/r${)}^{3/2}$], where ensuremath{iota} is the angle between the normal to the orbital plane and the spin direction, and ${mathrm{ensuremath{iota}}}_{0}$ is the initial value of ensuremath{iota}, when r is very large." @default.
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- W2045142020 date "1995-09-15" @default.
- W2045142020 modified "2023-09-26" @default.
- W2045142020 title "Effect of gravitational radiation reaction on circular orbits around a spinning black hole" @default.
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- W2045142020 doi "https://doi.org/10.1103/physrevd.52.r3159" @default.
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