The Near-Horizon Limit of the Extreme Rotating d=5 Black Hole as a Homogenous Spacetime

Details The Near-Horizon Limit of the Extreme Rotating d=5 Black Hole as a Homogenous Spacetime The Near-Horizon Limit of the Extreme Rotating d=5 Black Hole as a Homogenous Spacetime

2002-09-08

arxiv.org/abs/hep-th/0209069v2

Class.Quant.Grav. 20 (2003) 423-430

Physics

High Energy Physics

High Energy Physics - Theory

Some points clarified and misprints corrected. Version to be published in Classical and Quantum Gravity

Scientific paper

We show that the spacetime of the near-horizon limit of the extreme rotating d=5 black hole, which is maximally supersymmetric in N=2,d=5 supergravity for any value of the rotation parameter j in [-1,1], is locally isomorphic to a homogeneous non-symmetric spacetime corresponding to an element of the 1-parameter family of coset spaces SO(2,1)x SO(3)/SO(2)_j in which the subgroup SO(2)_j is a combination of the two SO(2) subgroups of SO(2,1) and SO(3).

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