Published February 7, 2003 | Version v1
Journal article

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

Description

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 element of [-1, 1], is locally isomorphic to a homogeneous non-symmetric spacetime corresponding to an element of the one-parameter family of coset spaces SO(2, 1)xSO(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)

Availability note (English)

Available online at http://stacks.iop.org/0264-9381/20/423/q30303.pdf or at the Web site for the journal Classical and Quantum Gravity (ISSN 1361-6382) http://www.iop.org/

Additional details

Identifiers

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
20
Journal Issue
3
Journal Page Range
p. 423-429
ISSN
0264-9381
CODEN
CQGRDG

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
34023130
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
BLACK HOLES; QUANTUM FIELD THEORY; SO GROUPS; SPACE-TIME; STRING MODELS; SUPERGRAVITY; SUPERSYMMETRY
Descriptors DEC
COMPOSITE MODELS; EXTENDED PARTICLE MODEL; FIELD THEORIES; LIE GROUPS; MATHEMATICAL MODELS; PARTICLE MODELS; QUARK MODEL; SYMMETRY; SYMMETRY GROUPS; UNIFIED-FIELD THEORIES