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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.
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Journal
Year
Volume
Issue
Pages
1173-1181
Physical description
Dates
published
1 - 10 - 2011
online
15 - 9 - 2011
Contributors
author
- Department of Physics, “Gh. Asachi” Technical University, Iasi, 700050, Romania
author
- Department of Civil Engineering, University of Thessaly, 383 34, Volos, Greece
author
- School of Applied Mathematics and Physical Sciences, National Technical University of Athens, 157 80, Athens, Greece
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Publication order reference
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YADDA identifier
bwmeta1.element.-psjd-doi-10_2478_s11534-011-0045-0