Published July 17, 2008
| Version v1
Journal article
Warm-Chaplygin inflationary universe model
Creators
- 1. Instituto de Fisica, Pontificia Universidad Catolica de Valparaiso, Casilla 4059, Valparaiso (Chile)
Description
Warm inflationary universe models in the context of a Chaplygin gas equation are studied. General conditions required for these models to be realizable are derived and discussed. By using a chaotic potential we develop models for a dissipation coefficient of the form Γ∝φn, with n=0 or n≠0
Availability note (English)
Available from http://dx.doi.org/10.1016/j.physletb.2008.05.063Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2008.05.063;
- arXiv
- arXiv:0806.0575v1;
- PII
- S0370-2693(08)00677-1;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 665
- Journal Issue
- 2-3
- Journal Page Range
- p. 100-105
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40046986
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- CHAOS THEORY; EQUATIONS; INFLATIONARY UNIVERSE; POTENTIALS
- Descriptors DEC
- COSMOLOGICAL MODELS; MATHEMATICAL MODELS; MATHEMATICS
Optional Information
- Copyright
- Copyright (c) 2008 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.