Published September 15, 2005
| Version v1
Journal article
Scale invariant hairy black holes
Creators
- 1. Departamento de Fisica, P. Universidad Catolica de Chile, Casilla 306, Santiago 22 (Chile)
- 2. Max-Planck-Institut fuer Gravitationsphysik, Albert-Einstein-Institut, 14476 Golm (Germany)
Description
Scalar fields coupled to three-dimensional gravity are considered. We uncover a scaling symmetry present in the black hole reduced action, and use it to prove a Smarr formula valid for any potential. We also prove that nonrotating hairy black holes exists only for positive total energy. The extension to higher dimensions is also considered
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.72.064019;
- arXiv
- arXiv:hep-th/0506025v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 72
- Journal Issue
- 6
- Journal Page Range
- p. 064019-064019.8
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37027609
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- BLACK HOLES; COSMOLOGY; GRAVITATION; POTENTIALS; SCALAR FIELDS; SYMMETRY; THREE-DIMENSIONAL CALCULATIONS
Optional Information
- Notes
- (c) 2005 The American Physical Society