Near Horizon Geometry and Black Holes in Four Dimensions

Details Near Horizon Geometry and Black Holes in Four Dimensions Near Horizon Geometry and Black Holes in Four Dimensions

1998-02-28

arxiv.org/abs/hep-th/9802198v3

Nucl.Phys. B528 (1998) 229-237

Physics

High Energy Physics

High Energy Physics - Theory

9 pages, LaTeX, small clarifications, references added, version to appear in Nucl. Phys. B

Scientific paper

10.1016/S0550-3213(98)00334-4

A large class of extremal and near-extremal four dimensional black holes in M-theory feature near horizon geometries that contain three dimensional asymptotically anti-de Sitter spaces. Globally, these geometries are derived from AdS_3 by discrete identifications. The microstates of such black holes can be counted by exploiting the conformal symmetry induced on the anti-de Sitter boundary, and the result agrees with the Bekenstein-Hawking area law. This approach, pioneered by Strominger, clarifies the physical nature of the black hole microstates. It also suggests that recent analyses of the relationship between boundary conformal field theory and supergravity can be extended to orbifolds of AdS spaces.

Affiliated with

Also associated with

No associations

Rating

Near Horizon Geometry and Black Holes in Four Dimensions 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 Near Horizon Geometry and Black Holes in Four Dimensions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near Horizon Geometry and Black Holes in Four Dimensions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-102965