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Prog. Theor. Phys. Vol. 99 No. 1 (1998) pp. 79-95
Regularization of Gravitational Radiation Reaction Force
Yasushi Mino*)
Department of Earth and Space Science,
Graduate School of Science
Osaka University, Toyonaka 560, Japan
and
Department of Physics,
Kyoto University, Kyoto 606-01, Japan
(Received October 20, 1997)
Abstract:
A particle with negligible mass is known
to move along a geodesic of a background spacetime.
We discuss the leading correction
to the equation of motion due to the mass of the particle
and its explicit derivation when the background metric
is a Schwarzschild/Kerr geometry.
This paper focuses on the metric perturbation
only around the particle and
proposes a new method to derive a finite radiation reaction force
to the particle motion.
An advantage of this method is that it is possible to
calculate the adiabatic evolution of all kinds of bound orbits.
In order to verify this method,
we consider the radiation reaction to a particle
in a circular orbit around a Schwarzschild black hole.
URL :
http://ptp.ipap.jp/link?PTP/99/79/
DOI : 10.1143/PTP.99.79
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Citing Article(s) :
-
Progress of Theoretical Physics Vol. 105 No. 2 (2001) pp. 197-218
:
-
The Gravitational Reaction Force on a Particle in the Schwarzschild Background
-
Hiroyuki Nakano and Misao Sasaki
-
Progress of Theoretical Physics Vol. 106 No. 2 (2001) pp. 339-362
:
-
Self-Force on a Scalar Charge in Circular Orbit around a Schwarzschild Black Hole
-
Hiroyuki Nakano, Yasushi Mino and Misao Sasaki
