Published November 9, 2006
| Version v1
Journal article
Dissipative Liouville cosmology: A case study
- 1. University of Athens, Physics Department, Nuclear and Particle Physics Section, GR157 71, Athens (Greece)
- 2. King's College London, Physics Department, Theoretical Physics, Strand WC2R 2LS (United Kingdom)
- 3. Academy of Athens, Division of Natural Sciences, 28 Panepistimiou Avenue, Athens 10679 (Greece)
- 4. Astroparticle Physics Group, Houston Advanced Research Center (HARC), Mitchell Campus, Woodlands, TX 77381 (United States)
- 5. George P. and Cynthia W. Mitchell Institute for Fundamental Physics, Texas A and M University, College Station, TX 77843 (United States)
Description
We consider solutions of the cosmological equations pertaining to a dissipative, dilaton-driven off-equilibrium Liouville cosmological model, which may describe the effective field theoretic limit of a non-critical string model of the Universe. The non-criticality may be the result of an early-era catastrophic cosmic event, such as a big-bang, brane-world collision, etc. The evolution of the various cosmological parameters of the model are obtained, and the effects of the dilaton and off-shell Liouville terms, including briefly those on relic densities, which distinguish the model from conventional cosmologies, are emphasised
Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2006.09.035;
- arXiv
- arXiv:hep-th/0605181v1;
- PII
- S0370-2693(06)01196-8;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 642
- Journal Issue
- 3
- Journal Page Range
- p. 179-186
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38076745
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BRANES; COSMOLOGICAL MODELS; COSMOLOGY; EQUATIONS; MATHEMATICAL EVOLUTION; MATHEMATICAL SOLUTIONS; STRING MODELS; UNIVERSE
- Descriptors DEC
- COMPOSITE MODELS; EVOLUTION; EXTENDED PARTICLE MODEL; MATHEMATICAL MODELS; PARTICLE MODELS; QUARK MODEL
Optional Information
- Copyright
- Copyright (c) 2006 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.