Making Anti-de Sitter Black Holes

Details Making Anti-de Sitter Black Holes Making Anti-de Sitter Black Holes

1996-04-02

arxiv.org/abs/gr-qc/9604005v1

Class.Quant.Grav. 13 (1996) 2707-2714

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

LaTeX, 10 pages, 6 postscript figures, uses epsf.tex

Scientific paper

10.1088/0264-9381/13/10/010

It is known from the work of Banados et al. that a space-time with event horizons (much like the Schwarzschild black hole) can be obtained from 2+1 dimensional anti-de Sitter space through a suitable identification of points. We point out that this can be done in 3+1 dimensions as well. In this way we obtain black holes with event horizons that are tori or Riemann surfaces of genus higher than one. They can have either one or two asymptotic regions. Locally, the space-time is isometric to anti-de Sitter space.

Affiliated with

Also associated with

No associations

Rating

Making Anti-de Sitter Black Holes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Making Anti-de Sitter Black Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Making Anti-de Sitter Black Holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-124019