Energy associated with a static spherically symmetric nonsingular black hole

Details Energy associated with a static spherically symmetric nonsingular black hole Energy associated with a static spherically symmetric nonsingular black hole

2001-08-27

arxiv.org/abs/gr-qc/0108067v1

Chin.J.Phys. 41 (2003) 326

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Scientific paper

We evaluate the energy distributions of the Dymnikova space-time using the Weinberg, Papapetrou, and M{\o}ller 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 M{\o}ller are not.

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