Exotic black hole solution in teleparallel theory of (2+1)-dimensional gravity

Details Exotic black hole solution in teleparallel theory of (2+1)-dimensional gravity Exotic black hole solution in teleparallel theory of (2+1)-dimensional gravity

1994-10-24

arxiv.org/abs/gr-qc/9410032v1

Prog.Theor.Phys. 94 (1995) 1169-1174

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

11, ReVTeX

Scientific paper

10.1143/PTP.94.1169

A black hole solution in a teleparallel theory of (2+1)-dimensional gravity, given in a previous paper, is examined. This solution is also a solution of the three-dimensional vacuum Einstein equation with a vanishing cosmological constant. Remarkable is the fact that this solution gives a black hole in a \lq \lq flat-land" in the Einstein theory and a Newtonian limit. Coordinate transformations to \lq \lq Minkowskian" coordinates, however, are singular not only at the origin, but also on the event horizon. {\em In the three-dimensional Einstein theory, vacuum regions of space-times can be locally non-trivial}.

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