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

• Authors: Irina Radinschi , Theophanes Grammenos , Andromahi Spanou
• Languages of publication: EN

Abstracts

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.

Keywords

EN

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

Discipline

• 04.20.-q: Classical general relativity(see also 02.40.-k Geometry, differential geometry, and topology)
• 04.20.Cv: Fundamental problems and general formalism
• 04.70.-s: Physics of black holes(see also 97.60.Lf—in astronomy)

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2011
• Volume: 9
• Issue: 5
• Pages: 1173-1181

Dates

published

1 - 10 - 2011

online

15 - 9 - 2011

Contributors

author

Irina Radinschi

• Department of Physics, “Gh. Asachi” Technical University, Iasi, 700050, Romania

author

Theophanes Grammenos

• Department of Civil Engineering, University of Thessaly, 383 34, Volos, Greece

author

Andromahi Spanou

• School of Applied Mathematics and Physical Sciences, National Technical University of Athens, 157 80, Athens, Greece

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Identifiers

DOI

10.2478/s11534-011-0045-0