The near-horizon limit of the extreme rotating d 5 black hole as a homogeneous spacetime

DOI10.1088/0264-9381/20/3/303zbMath1054.83017arXivhep-th/0209069OpenAlexW1992965519MaRDI QIDQ4808039

Natxo Alonso-Alberca, Tomás Ortín, Ernesto Lozano-Tellechea

Publication date: 14 July 2003

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0209069

zbMATH Keywords

supergravityblack hole spacetime

Mathematics Subject Classification ID

Black holes (83C57) Supergravity (83E50) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)

Related Items

Microscopic realization of the Kerr/CFT correspondence, Classification of maximally supersymmetric backgrounds in supergravity theories, Spinning deformations of the D1-D5 system and a geometric resolution of closed timelike curves, Supersymmetric probes in a rotating 5D attractor, Emergent \(\mathrm{AdS}_{3}\) in the zero entropy extremal black holes