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

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dc.creatorHayward, Sean A.
dc.date2000-12-20
dc.date2001-02-05
dc.date.accessioned2026-07-07T03:25:31Z
dc.date.available2026-07-07T03:25:31Z
dc.descriptionGravitational 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.
dc.description4 revtex pages, stresses radiation rather than waves
dc.identifierhttps://arxiv.org/abs/gr-qc/0012077
dc.identifierhttp://arxiv.org/abs/gr-qc/0012077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33742
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational radiation, energy and reaction on quasi-spherical black holes
dc.typetext

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