Gravitational Radiation from a Kerr Black Hole. I ---Formulation and a Method for Numerical Analysis---

Details Gravitational Radiation from a Kerr Black Hole. I ---Formulation and a Method for Numerical Analysis--- Gravitational Radiation from a Kerr Black Hole. I ---Formulation and a Method for Numerical Analysis---

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pthph..67.1788s&link_type=abstract

Progress of Theoretical Physics, Vol. 67, No. 6, pp. 1788-1809

Physics

81

Scientific paper

A class of new inhomogeneous equations governing gravitational perturbations of the Kerr geometry is presented. It is shown that, contrary to the case of the Teukolsky equation, the perturbation equations have short-range potential and no divergent source terms for large distance. Using one of such equations which seems to be the simplest, we have computed the spectrum and the energy ofgravitational radiation induced by a test particle of mass μ falling along the z-axis into a Kerr black hole of mass M(≫μ) and angular momentum Ma(a

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