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

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

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pthph..66.1627r&link_type=abstract

Progress of Theoretical Physics, Vol. 66, No. 5, pp. 1627-1638

Physics

18

Scientific paper

A semi-relativistic treatment estimating the gravitational radiation emitted by a particle thrusted into a Schwarzschil 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.

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