Energy associated with a static spherically symmetric nonsingular black hole

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dc.creatorYang, I-Ching
dc.creatorRadinschi, Irina
dc.date2001-08-27
dc.date.accessioned2026-07-25T17:02:22Z
dc.descriptionWe evaluate the energy distributions of the Dymnikova space-time using the Weinberg, Papapetrou, and Møller energy-momentum complexes. This result sustain the importance of the energy-momentum complexes in the evaluation of the energy distribution of a given space-time. To compare the energy distributions obtained by using several definitions, these results show that the Einstein, Tolman, and Weinberg energy complexes are the same in Schwarzschild Cartesian coordinates, but the Papapetrou and the Møller are not.
dc.identifierhttps://arxiv.org/abs/gr-qc/0108067
dc.identifierhttp://arxiv.org/abs/gr-qc/0108067
dc.identifierChin.J.Phys. 41 (2003) 326
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/45190
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEnergy associated with a static spherically symmetric nonsingular black hole
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