Energy Distribution in a Schwarzschild-like Spacetime

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dc.creatorGrammenos, Th.
dc.creatorRadinschi, I.
dc.date2006-02-25
dc.date2006-08-02
dc.date.accessioned2026-07-07T10:28:15Z
dc.date.available2026-07-07T10:28:15Z
dc.descriptionIn this paper, utilizing Møller's energy-momentum complex, we explicitly evaluate the energy and momentum density associated with a metric describing a four-dimensional, Schwarzschild-like, spacetime derived from an effective gravity coupled with a U(1) gauge field in the context of a D3-brane dynamics in the classical regime, i.e., between the asymptotic and the Planck regime.
dc.description10 pages; title changed; references updated; content revised
dc.identifierhttps://arxiv.org/abs/gr-qc/0602105
dc.identifierhttp://arxiv.org/abs/gr-qc/0602105
dc.identifierInt.J.Theor.Phys.46:1055-1064,2007
dc.identifierdoi:10.1007/s10773-006-9259-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177385
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEnergy Distribution in a Schwarzschild-like Spacetime
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