Energy distribution in a BTZ black hole spacetime

Abstract

We evaluate the energy distribution associated with the (2+1)-dimensional rotating BTZ black hole. The energy-momentum complexes of Landau-Lifshitz and Weinberg are employed for this computation. Both prescriptions give exactly the same form of energy distribution. Therefore, these results provide evidence in support of the claim that, for a given gravitational background, different energy-momentum complexes can give identical results in three dimensions, as it is the case in four dimensions.

16 pages, LaTeX; v2: comments, clarifications and references added, version to appear in Int.J.Mod.Phys.D

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