Adiabatic radiation reaction to the orbits in Kerr Spacetime

Details Adiabatic radiation reaction to the orbits in Kerr Spacetime Adiabatic radiation reaction to the orbits in Kerr Spacetime

2005-06-17

arxiv.org/abs/gr-qc/0506092v1

Prog.Theor.Phys. 114 (2005) 509-514

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5pages, no figure, accepted for publication in PTP

Scientific paper

10.1143/PTP.114.509

Geodesic motion of a point particle in Kerr geometry has three constants of
motion, energy $E$, azimuthal angular momentum $L$, and Carter constant $Q$.
Under the adiabatic approximation, radiation reaction effect is characterized
by the time evolution of these constants. In this letter we show that the
scheme to evaluate them can be dramatically simplified.

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