Gravitational radiation from dynamical black holes

Details Gravitational radiation from dynamical black holes Gravitational radiation from dynamical black holes

2005-05-16

arxiv.org/abs/gr-qc/0505080v2

Class.Quant.Grav. 23 (2006) L15

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 revtex4 pages. Additional comments

Scientific paper

10.1088/0264-9381/23/3/L01

An effective energy tensor for gravitational radiation is identified for uniformly expanding flows of the Hawking mass-energy. It appears in an energy conservation law expressing the change in mass due to the energy densities of matter and gravitational radiation, with respect to a Killing-like vector encoding a preferred flow of time outside a black hole. In a spin-coefficient formulation, the components of the effective energy tensor can be understood as the energy densities of ingoing and outgoing, transverse and longitudinal gravitational radiation. By anchoring the flow to the trapping horizon of a black hole in a given sequence of spatial hypersurfaces, there is a locally unique flow and a measure of gravitational radiation in the strong-field regime.

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