Gravitational radiation, energy and reaction on quasi-spherical black holes

Details Gravitational radiation, energy and reaction on quasi-spherical black holes Gravitational radiation, energy and reaction on quasi-spherical black holes

2000-12-20

arxiv.org/abs/gr-qc/0012077v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 revtex pages, stresses radiation rather than waves

Scientific paper

Gravitational radiation is locally defined where the wavefronts are roughly spherical. A local energy tensor is defined for the gravitational radiation. Including this energy tensor as a source in the truncated Einstein equations describes gravitational radiation reaction, such as back-reaction on a roughly spherical black hole. The energy-momentum in a canonical frame is covariantly conserved. The strain to be measured by a distant detector is simply defined.

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