2008/04/22 by R. F. ARANHA, R. F. Aranha, H. P. de Oliveira +5 · 1 citation
Engineering · Physics and Astronomy · #Pulsars and Gravitational Waves Research #Statistical Mechanics and Entropy #Thermoelastic and Magnetoelastic Phenomena #gr-qc
paper · pdf · doi:10.1142/s0218271808013704
published as Int.J.Mod.Phys.D17:2049-2064,2008 · 16 pages, 4 figures, to appear in Int. J. Modern Phys. D (2008)
arxiv created 2008/04/22 · openalex publication_date 2008/10/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
In this paper, we examine the efficiency of gravitational bremsstrahlung production in the process of head-on collision of two boosted Schwarzschild black holes. We construct initial data for the characteristic initial value problem in Robinson–Trautman space–times, which represent two instantaneously stationary Schwarzschild black holes in motion toward each other with the same velocity. The Robinson–Trautman equation is integrated for these initial data using a numerical code based on the Galerkin method. The resulting final configuration is a boosted black hole with Bondi mass greater than the sum of the individual masses of the individual initial black holes. Two relevant aspects of the process are presented. The first relates the efficiency Δ of the energy extraction by gravitational wave emission to the mass of the final black hole. This relation is fitted by a distribution function of nonextensive thermostatistics with entropic parameter q ≃ 1/2; the result extends and validates analysis based on the linearized theory of gravitational wave emission. The second aspect is a typical bremsstrahlung angular pattern in the early period of emission at the wave zone, a consequence of the deceleration of the black holes as they coalesce; this pattern evolves to a quadrupole form for later times.