中文

Cosmology with a Variable Chaplygin Gas

天体物理学 2008-11-26 v3 广义相对论与量子宇宙学 高能物理 - 唯象学

摘要

We consider a new generalized Chaplygin gas model that includes the original Chaplygin gas model as a special case. In such a model the generalized Chaplygin gas evolves as from dust to quiessence or phantom. We show that the background evolution for the model is equivalent to that for a coupled dark energy model with dark matter. The constraints from the current type Ia supernova data favour a phantom-like Chaplygin gas model.

引用

@article{arxiv.astro-ph/0506091,
  title  = {Cosmology with a Variable Chaplygin Gas},
  author = {Zong-Kuan Guo and Yuan-Zhong Zhang},
  journal= {arXiv preprint arXiv:astro-ph/0506091},
  year   = {2008}
}

备注

8 pages, 3 figures, LaTeX2e, Accepted for publication in Phys. Lett. B