Abstract
We present a class of solutions to the Einstein–Maxwell equations in d-dimensions, all of which are asymptotically (anti)-de Sitter spacetimes. They describe electrically charged rotating solutions, which are generalizations of those found by Lemos (1994 Preprint 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.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.