Closed timelike curves in asymmetrically warped brane universes
- 1. Fakutaet fuer Physik, Technische Universitaet Dortmund, D-44221 Dortmund (Germany)
- 2. Department of Physics and Astronomy, University of Hawaii at Manoa, 2505 Correa Road, Honolulu, Hawaii 96822 (United States)
- 3. Department of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235 (United States)
Description
In asymmetrically-warped spacetimes different warp factors are assigned to space and to time. We discuss causality properties of these warped brane universes and argue that scenarios with two extra dimensions may allow for timelike curves which can be closed via paths in the extra-dimensional bulk. In particular, necessary and sufficient conditions on the metric for the existence of closed timelike curves are presented. We find a six-dimensional warped metric which satisfies the CTC conditions, and where the null, weak and dominant energy conditions are satisfied on the brane (although only the former remains satisfied in the bulk). Such scenarios are interesting, since they open the possibility of experimentally testing the chronology protection conjecture by manipulating on our brane initial conditions of gravitons or hypothetical gauge-singlet fermions (''sterile neutrinos'') which then propagate in the extra dimensions.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.80.044008;
- arXiv
- arXiv:gr-qc/0603045v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 80
- Journal Issue
- 4
- Journal Page Range
- p. 044008-044008.11
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41063590
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CAUSALITY; GRAVITONS; METRICS; NEUTRINOS; SPACE-TIME; UNIVERSE
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; GRAVITATIONAL RADIATION; LEPTONS; MASSLESS PARTICLES; POSTULATED PARTICLES; RADIATIONS
Optional Information
- Notes
- (c) 2009 The American Physical Society