Static axisymmetric approach for the head-on collision of two black holes

Details Static axisymmetric approach for the head-on collision of two black holes Static axisymmetric approach for the head-on collision of two black holes

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvd..52..816a&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 52, Issue 2, 15 July 1995, pp.816-820

Physics

6

Approximation Methods, Equations Of Motion, Gravitational Waves: Theory, Classical Black Holes, Black Holes

Scientific paper

This paper presents a semianalytical approach to the interaction of two (originally) spherically symmetric black holes through a head-on collision process. It is shown that an expression for the rate of emission of gravitational radiation can be derived from the so-called Weyl potential. The total output of gravitational wave energy released is then calculated and the results are compared to recent numerical investigations of this problem.

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