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| DOI | 10.1016/J.PHYSLETB.2017.03.065 | ||||
| Año | 2017 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
In this paper we present a phantom solution with a big rip singularity in a non-linear regime of the Israel-Stewart formalism. In this framework it is possible to extend this causal formalism in order to describe accelerated expansion, where assumption of near equilibrium is no longer valid. We assume a flat universe filled with a single viscous fluid ruled by a barotropic EoS, p = omega rho, which can represent a late time accelerated phase of the cosmic evolution. The solution allows to cross the phantom divide without evoking an exotic matter fluid and the effective EoS parameter is always lesser than -1 and constant in time. (C) 2017 The Authors. Published by Elsevier B.V.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Cruz, Miguel | Hombre |
Univ Veracruzana - México
Universidad Veracruzana - México |
| 2 | Cruz, Norman | Hombre |
Universidad de Santiago de Chile - Chile
|
| 3 | LEPE-SANTA CRUZ, SAMUEL | Hombre |
Pontificia Universidad Católica de Valparaíso - Chile
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| Fuente |
|---|
| Consejo Nacional de Ciencia y Tecnología |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Comisión Nacional de Investigación Científica y Tecnológica |
| Pontificia Universidad Católica de Valparaíso |
| Sistema Nacional de Investigadores |
| Comisión Nacional de Investigación CientÃfica y Tecnológica |
| Pontificia Universidad Cat?lica de Valpara?so |
| Fondo Nacional de Desarrollo CientÃfico, Tecnológico y de Innovación Tecnológica |
| Chilean Institutions: CONICYT, through the Fondecyt |
| CONACyT-Mexico through the grant Repatriaciones, cuarta fase and SNI |
| Pontificia Universidad Catolica de Valparaiso, Chile, through the VRIEA-DI-PUCV grant |
| CONACyT-M? |
| VRIEA-DI-PUCV |
| California Health Care Safety Net Institute |
| Agradecimiento |
|---|
| N. C. acknowledges the hospitality of the Facultad de Fisica of Universidad Veracruzana, Mexico, where part of this work was done. This work has been supported by CONACyT-Mexico through the grant Repatriaciones, 2015, cuarta fase and SNI (M. C.) and N. C. and S. L. acknowledge the support of following Chilean Institutions: CONICYT, through the Fondecyt grant No. 1140238 (N. C.) and Pontificia Universidad Catolica de Valparaiso, Chile, through the VRIEA-DI-PUCV grant No. 039.351/2016 (S. L.) |
| N. C. acknowledges the hospitality of the Facultad de Física of Universidad Veracruzana, México, where part of this work was done. This work has been supported by CONACyT-México through the grant Repatriaciones, 2015, cuarta fase and SNI (M. C.) and N. C. and S. L. acknowledge the support of following Chilean Institutions: CONICYT, through the Fondecyt grant No. 1140238 (N. C.) and Pontificia Universidad Católica de Valparaíso, Chile, through the VRIEA-DI-PUCV grant No. 039.351/2016 (S. L.). |