Abstract
In this work we have derived a class of geometries which describe black holes and wormholes in Randall-Sundrum–type brane models, focusing mainly on asymptotically anti-de Sitter backgrounds. We show that by continuously deforming the usual four-dimensional vacuum background, a specific family of solutions is obtained. Maximal extensions of the solutions are presented, and their causal structures are discussed.
- Received 12 May 2010
DOI:https://doi.org/10.1103/PhysRevD.82.044029
© 2010 The American Physical Society
