Higher Dimensional Charged Rotating Solutions in (A)dS Space-times

Abstract

We present a class of solutions to the Einstein-Maxwell equations in d-dimensions, all of which are asymptotically (anti)-de Sitter space-times. They describe electrically charged rotating solutions, which are generalizations of those found by Lemos (gr-qc/9404041). These solutions have toroidal, planar or cylindrical horizons and can be interpreted as black holes, or black strings/branes. We calculate the inverse temperature and entropy, and then we use the Brown-York stress-tensor to calculate mass and angular momenta of these solutions.

7+1 pages, LateX2e(v3: a discussion on horizons and singularities have been added as well as few references)

References in corpus (3)

• Quasi-normal modes of toroidal, cylindrical and planar black holes in anti-de Sitter spacetimes: scalar, electromagnetic and gravitational perturbations
• Stable Black Strings in Anti-de Sitter Space
• Supersymmetry of the extreme rotating toroidal black hole

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