Effective mass of a radiating charged particle in Einstein's universe

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dc.creatorVagenas, Elias C.
dc.date2003-11-06
dc.date2003-12-17
dc.date.accessioned2026-07-07T10:29:58Z
dc.date.available2026-07-07T10:29:58Z
dc.descriptionThe effective gravitational mass as well as the energy and momentum distributions of a radiating charged particle in Einstein's universe are evaluated. The Moller's energy-momentum complex is employed for this computation. The spacetime under study is a generalization of Bonnor and Vaidya spacetime in the sense that the metric is described in the cosmological background of Einstein's universe in lieu of the flat background. Several spacetimes are limiting cases of the one considered here. Particularly for the Reissner-Nordstrom black hole background, our results are exactly the same with those derived by Cohen and Gautreau using Whittaker's theorem and by Cohen and de Felice using Komar's mass. Furthermore, the power output for the spacetime under consideration is obtained.
dc.description12 pages, LaTeX; to appear in Mod.Phys.Lett.A
dc.identifierhttps://arxiv.org/abs/hep-th/0311050
dc.identifierhttp://arxiv.org/abs/hep-th/0311050
dc.identifierMod.Phys.Lett.A19:213-222,2004
dc.identifierdoi:10.1142/S0217732304015671
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177994
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEffective mass of a radiating charged particle in Einstein's universe
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