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Open Physics

formerly Central European Journal of Physics

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Volume 9, Issue 5

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Localization of energy for a regular black hole solution in an asymptotically de Sitter spacetime geometry

Irina Radinschi / Theophanes Grammenos / Andromahi Spanou
  • School of Applied Mathematics and Physical Sciences, National Technical University of Athens, 157 80, Athens, Greece
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Published Online: 2011-09-15 | DOI: https://doi.org/10.2478/s11534-011-0045-0

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Abstract

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.

PACS: 04.20.-q; 04.20.Cv; 04.70.-s

Keywords: energy-momentum complexes; regular black holes; asymptotically de Sitter spacetime

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About the article

Published Online: 2011-09-15

Published in Print: 2011-10-01

Citation Information: Open Physics, Volume 9, Issue 5, Pages 1173–1181, ISSN (Online) 2391-5471, DOI: https://doi.org/10.2478/s11534-011-0045-0.

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