Power-law tail of gravitational waves from a uniformly accelerating black hole

Details Power-law tail of gravitational waves from a uniformly accelerating black hole Power-law tail of gravitational waves from a uniformly accelerating black hole

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvd..57.2613t&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 57, Issue 4, 15 February 1998, pp.2613-2616

Physics

4

Wave Generation And Sources, Classical Black Holes

Scientific paper

To investigate the late-time behavior of gravitational waves at future null infinity, we reexamine the vacuum C-metric describing a uniformly accelerating Schwarzschild black hole. By using the mass function defined in the Bondi-Metzner-Sachs coordinate system, it is clearly shown that the power-law tail predicted by linearized perturbation theory develops also in this fully nonlinear axisymmetric dynamics.

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