A Radiating and Rotating Metric

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dc.creatorWagh, Sanjay M.
dc.creatorMuktibodh, Pradeep S.
dc.date1999-02-23
dc.date.accessioned2026-07-07T03:32:59Z
dc.date.available2026-07-07T03:32:59Z
dc.descriptionA non-static solution of Einstein's field equations of General Relativity representing the gravitational field of an axisymmetric radiation flow is obtained using the Eddington or the Kerr-Schild form for the metric. A solution obtained here manifestly corresponds to the Kerr metric with its mass-parameter, $m$, being an arbitrary function of the advanced (retarded) null-time coordinate. Then, when $m$ is constant, the solution reduces to the standard Kerr metric expressed in terms of the used null coordinate. Further, when the angular momentum parameter, $a$, a constant here, is set to zero, the solution reduces to the Vaidya metric expressed in terms of the used null-coordinate.
dc.descriptionLatex file 11 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9902071
dc.identifierhttp://arxiv.org/abs/gr-qc/9902071
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36447
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA Radiating and Rotating Metric
dc.typetext

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