Energy Distribution of a Charged Black Hole with a Minimally Coupled Scalar Field

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dc.creatorHalpern, Paul
dc.date2007-05-05
dc.date2007-11-01
dc.date.accessioned2026-07-07T11:20:30Z
dc.date.available2026-07-07T11:20:30Z
dc.descriptionUsing three different energy-momentum complexes, the Einstein, Landau-Lifshitz, and Papapetrou prescriptions, we calculate the energy of an electrically charged black hole exact solution with a self-interacting, minimally-coupled scalar field and the asymptotic region locally an Anti-deSitter spacetime. Writing the metric in Kerr-Schild Cartesian coordinates, we demonstrate that this metric belongs to the Kerr-Schild class of solutions. Applying each of the three energy-momentum prescriptions and comparing the results, we find consistency among these complexes, suggesting their utility as localized measures of energy.
dc.description11 pages; To appear in Astrophysics and Space Science
dc.identifierhttps://arxiv.org/abs/0705.0720
dc.identifierhttp://arxiv.org/abs/0705.0720
dc.identifierAstrophys.SpaceSci.313:357-361,2008
dc.identifierdoi:10.1007/s10509-007-9704-4
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193982
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleEnergy Distribution of a Charged Black Hole with a Minimally Coupled Scalar Field
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