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

Abstract

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).

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

References in corpus (7)

• Black Holes of D=5 Supergravity
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• Microscopic Realization of the Kerr/CFT Correspondence
• Statistical Description of Rotating Kaluza-Klein Black Holes
• Supergravity vacua and lorentzian Lie groups
• Emergent AdS_3 in the Zero Entropy Extremal Black Holes
• Supersymmetric Probes in a Rotating 5D Attractor
• Wrapped M2/M5 Duality
• Causal Structure of d=5 Vacua and Axisymmetric Spacetimes
• The Spectra of Supersymmetric States in String Theory
• All-order consistency of 5d sugra vacua
• Classification of maximally supersymmetric backgrounds in supergravity theories
• More Bubbling Solutions
• Near horizon superconformal symmetry of rotating BPS black holes in five dimensions