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Note on regular black holes in a brane world

Published 14 Aug 2015 in gr-qc, astro-ph.HE, and hep-th | (1508.03615v2)

Abstract: In this work, we show that regular black holes in a Randall-Sundrum-type brane world model are generated by the nonlocal bulk influence, expressed by a constant parameter in the brane metric, only in the spherical case. In the axial case (black holes with rotation), this influence forbids them. A nonconstant bulk influence is necessary to generate regular black holes with rotation in this context.

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