Published November 10, 2014
| Version v1
Journal article
The BTZ black hole as a Lorentz-flat geometry
Creators
- 1. Rudolf Peierls Centre for Theoretical Physics, University of Oxford (United Kingdom)
- 2. Universidad Andrés Bello, Av. República 440, Santiago (Chile)
- 3. Centro de Estudios Científicos (CECs), Av. Arturo Prat 514, Valdivia (Chile)
- 4. Departamento de Matemática y Física Aplicadas, Universidad Católica de la Santísima Concepción, Concepción (Chile)
- 5. Physique Théorique et Mathématique, Université Libre de Bruxelles and International Solvay Institutes, Campus Plaine C.P. 231, B-1050 Bruxelles (Belgium)
- 6. Departamento de Física, Universidad de Concepción, Casilla 160-C, Concepción (Chile)
Description
It is shown that 2+1 dimensional anti-de Sitter spacetimes are Lorentz-flat. This means, in particular, that any simply-connected patch of the BTZ black hole solution can be endowed with a Lorentz connection that is locally pure gauge. The result can be naturally extended to a wider class of black hole geometries and point particles in three-dimensional spacetime
Availability note (English)
Available from http://dx.doi.org/10.1016/j.physletb.2014.09.032Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2014.09.032;
- arXiv
- arXiv:1405.6657v1;
- PII
- S0370-2693(14)00682-0;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 738
- Journal Page Range
- p. 134-135
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 47003952
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANTI DE SITTER SPACE; BLACK HOLES; GAUGE INVARIANCE; MATHEMATICAL SOLUTIONS; PARTICLES; SPACE-TIME; THREE-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- INVARIANCE PRINCIPLES; MATHEMATICAL SPACE; SPACE
Optional Information
- Copyright
- Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.