Black Holes, Dark Wormholes and Solitons in f(T) Gravities
arXiv:1704.05919 · doi:10.1103/PhysRevD.95.124024
Abstract
By choosing an appropriate vielbein basis, we obtain a class of spherically-symmetric solutions in gravities. The solutions are asymptotic to Minkowski spacetimes with leading falloffs the same as those of the Schwarzschild black hole. In general, these solutions have branch-cut singularities in the middle. For appropriately chosen functions, extremal black holes can also emerge. Furthermore, we obtain wormhole configurations whose spatial section is analogous to an Ellis wormhole, but runs from 0 to 1 as the proper radial coordinate runs from to . Thus a signal sent from to through the wormhole will be infinitely red-shifted. We call such a spacetime configuration a dark wormhole. By introducing a bare cosmological constant , we construct smooth solitons that are asymptotic to local AdS with an effective . In the middle of bulk, the soliton metric behaves like the AdS of bare in global coordinates. We also embed AdS planar and Lifshitz black holes in gravities. Finally we couple the Maxwell field to the theories and construct electrically-charged solutions.
Latex, 31 pages, 2 figures, typos corrected and a reference added
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