Dissipative generalized Chaplygin gas as phantom dark energy
Abstract
The generalized Chaplygin gas, characterized by the equation of state p = - A / Ïα, has been considered as a model for dark energy due to its dark-energy-like evolution at late times. When dissipative processes are taken into account, within the framework of the standard Eckart theory of relativistic irreversible thermodynamics, cosmological analytical solutions are found. Using the truncated causal version of the Israel-Stewart formalism, a suitable model was constructed which crosses the w = - 1 barrier. The future-singularities encountered in both approaches are of a new type, and not included in the classification presented by Nojiri and Odintsov [S. Nojiri, S.D. Odintsov, Phys. Rev. D 72 (2005) 023003]. © 2007.
Más información
Título según WOS: | Dissipative generalized Chaplygin gas as phantom dark energy |
Título según SCOPUS: | Dissipative generalized Chaplygin gas as phantom dark energy |
Título de la Revista: | PHYSICS LETTERS B |
Volumen: | 646 |
Número: | 4 |
Editorial: | ELSEVIER SCIENCE BV |
Fecha de publicación: | 2007 |
Página de inicio: | 177 |
Página final: | 182 |
Idioma: | English |
URL: | http://linkinghub.elsevier.com/retrieve/pii/S0370269307000731 |
DOI: |
10.1016/j.physletb.2006.12.070 |
Notas: | ISI, SCOPUS |