Anti-de Sitter Quotients, Bubbles of Nothing, and Black Holes
High Energy Physics - Theory
2008-12-18 v2
Abstract
In 3+1 dimensions there are anti-de quotients which are black holes with toroidal event horizons. By analytic continuation of the Schwarzschild-anti-de Sitter solution (and appropriate identifications) one finds two one parameter families of spacetimes that contain these quotient black holes. One of these families consists of B-metrics ("bubbles of nothing"), the other of black hole spacetimes. All of them have vanishing conserved charges.
Keywords
Cite
@article{arxiv.0801.4214,
title = {Anti-de Sitter Quotients, Bubbles of Nothing, and Black Holes},
author = {Jan E. Aman and Stefan Aminneborg and Ingemar Bengtsson and Narit Pidokrajt},
journal= {arXiv preprint arXiv:0801.4214},
year = {2008}
}
Comments
14 pages, 3 figures. References added, one explanation improved