Multi-Black-Holes in 3D and 4D anti-de Sitter Spacetimes

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Talk given at the Journees Relativistes 96 (Ascona, Switzerland). 4 pages, LaTeX, includes 1 LaTeX figure

Scientific paper

The (single) black hole solutions of Ba\~nados, Teitelboim and Zanelli (BTZ) in 2+1 dimensional anti-de Sitter space are generalized to an arbitrary number $n$ of such black holes. The resulting multi-black-hole (MBH) spacetime is locally isometric to anti-de Sitter space, and globally it is obtained from the latter as a quotient space by means of suitable identifications. The MBH spacetime has $n$ asymptotically anti-de Sitter exterior regions, each of which has the geometry of a single BTZ black hole. These exterior regions are separated by $n$ horizons from a common interior region. This interior region can be described as a ``closed" universe containing $n$ black holes. Similar configurations in 3+1 dimensions, with horizons of toroidal and higher genus topologies, are also presented.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Multi-Black-Holes in 3D and 4D anti-de Sitter Spacetimes 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 Multi-Black-Holes in 3D and 4D anti-de Sitter Spacetimes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multi-Black-Holes in 3D and 4D anti-de Sitter Spacetimes will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-276986

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.