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2011 | 9 | 5 | 1173-1181
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Localization of energy for a regular black hole solution in an asymptotically de Sitter spacetime geometry

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EN
The energy and momentum distributions of a regular black hole in a four-dimensional, asymptotically de Sitter spacetime geometry are computed, whereby the Einstein, Landau-Lifshitz, Weinberg and Møller energy-momentum complexes are utilized. It is found, for all prescriptions applied, that the momentum distribution vanishes, while the energy distribution depends on the mass parameter M, the electric charge Q, and the cosmological constant Λ. In addition, various limiting cases are discussed.
Contributors
  • Department of Physics, “Gh. Asachi” Technical University, Iasi, 700050, Romania, radinschi@yahoo.com
  • Department of Civil Engineering, University of Thessaly, 383 34, Volos, Greece, thgramme@uth.gr
  • School of Applied Mathematics and Physical Sciences, National Technical University of Athens, 157 80, Athens, Greece, aspanou@central.ntua.gr
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YADDA identifier
bwmeta1.element.-psjd-doi-10_2478_s11534-011-0045-0
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