Simple Search:

Interacting two-fluid viscous dark energy models in a non-flat universe


Citation

Amirhashchi, Hassan and Pradhan, Anirudh and Zainuddin, Hishamuddin (2013) Interacting two-fluid viscous dark energy models in a non-flat universe. Research in Astronomy and Astrophysic, 13 (2). pp. 129-138. ISSN 1674-4527

Abstract / Synopsis

We study the evolution of the dark energy parameter within the scope of a spatially non-flat and isotropic Friedmann-Robertson-Walker model filled with barotropic fluid and bulk viscous stresses. We have obtained cosmological solutions that do not have a Big Rip singularity, and concluded that in both non-interacting and interacting cases the non-flat open Universe crosses the phantom region. We find that during the evolution of the Universe, the equation of state for dark energy ωD changes from ω eff D > -1 to ωeff D < -1, which is consistent with recent observations.


Download File

[img]
Preview
PDF (Abstract)
Interacting two.pdf

Download (178kB) | Preview

Additional Metadata

Item Type: Article
Divisions: Institute for Mathematical Research
DOI Number: https://doi.org/10.1088/1674-4527/13/2/001
Publisher: Institute of Physics Publishing
Keywords: Cosmology; Dark energy; Theory; Viscous fluid.
Depositing User: Umikalthom Abdullah
Date Deposited: 25 Jun 2014 04:07
Last Modified: 08 Sep 2015 01:24
Altmetrics: http://www.altmetric.com/details.php?domain=psasir.upm.edu.my&doi=10.1088/1674-4527/13/2/001
URI: http://psasir.upm.edu.my/id/eprint/30082
Statistic Details: View Download Statistic

Actions (login required)

View Item View Item