On a Semi-Relativistic Treatment of the Gravitational Radiation from a Mass Thrusted into a Black Hole

概要

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A semi-relativistic treatment estimating the gravitational radiation emitted by a particle thrusted into a Schwarzschild black hole with a finite kinetic energy at infinity is presented on the two extreme assumptions : (a) The particle moves along a geodesic in a curved space and (b) the particle radiates as if it were in flat space-time. The structure of the burst and beaming process of gravitational radiation are studied. The merit of this approach lies in its simplicity and in providing a direct and complementary understanding of the results obtained by a fully relativistic treatment.
理論物理学刊行会の論文
1981-11-25