Energy associated with a static spherically symmetric nonsingular black hole
Abstract
We evaluate the energy distributions of the Dymnikova space-time using the Weinberg, Papapetrou, and Mller 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 Mller are not.
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