Samiksha Jaiswal (Editor)

AdS black hole

Updated on
Edit
Like
Comment
Share on FacebookTweet on TwitterShare on LinkedInShare on Reddit

In theoretical physics, an AdS black hole is a black hole solution of general relativity or its extensions which represents an isolated massive object, but with a negative cosmological constant. Such a solution asymptotically approaches anti-de Sitter space at spatial infinity, and is a generalization of the Kerr vacuum solution, which asymptotically approaches Minkowski spacetime at spatial infinity.

In 3+1 dimensions, the metric is given by

d s 2 = ( k 2 r 2 + 1 C r ) d t 2 + 1 k 2 r 2 + 1 C r d r 2 + r 2 d Ω 2

where t is the time coordinate, r is the radial coordinate, Ω are the polar coordinates, C is a constant and k is the AdS curvature.

In general, in d+1 dimensions, the metric is given by

d s 2 = ( k 2 r 2 + 1 C r d 2 ) d t 2 + 1 k 2 r 2 + 1 C r d 2 d r 2 + r 2 d Ω 2

According to the AdS/CFT correspondence, if gravity were quantized, an AdS black hole would be dual to a thermal state on the conformal boundary. In the context of say, AdS/QCD, this would correspond to the deconfinement phase of the quark–gluon plasma.

References

AdS black hole Wikipedia