English

Interacting generalized Chaplygin gas model in non-flat universe

General Relativity and Quantum Cosmology 2010-10-27 v1

Abstract

We employ the generalized Chaplygin gas of interacting dark energy to obtain the equation of state for the generalized Chaplygin gas energy density in non-flat universe. By choosing a negative value for BB we see that wΛeff<1w_{\rm \Lambda}^{eff}< -1, that corresponds to a universe dominated by phantom dark energy.

Keywords

Cite

@article{arxiv.0711.0524,
  title  = {Interacting generalized Chaplygin gas model in non-flat universe},
  author = {M R Setare},
  journal= {arXiv preprint arXiv:0711.0524},
  year   = {2010}
}

Comments

8 pages, no figure

R2 v1 2026-06-21T09:39:38.909Z