Interacting Chaplygin gas

Hongsheng Zhang and Zong-Hong Zhu
Phys. Rev. D 73, 043518 – Published 23 February 2006

Abstract

We investigate a kind of interacting Chaplygin gas model in which the Chaplygin gas plays the role of dark energy and interacts with cold dark matter particles. We find that there exists a stable scaling solution at late times with the Universe evolving into a phase of steady state. Furthermore, the effective equation of state of Chaplygin gas may cross the so-called phantom divide w=1. The above results are derived from continuity equations, which means that they are independent of any gravity theories. Assuming standard general relativity and a spatially flat Friedamnn-Robertson-Walker (FRW) metric, we also find the deceleration parameter is well consistent with current observations.

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  • Received 30 September 2005

DOI:https://doi.org/10.1103/PhysRevD.73.043518

©2006 American Physical Society

Authors & Affiliations

Hongsheng Zhang* and Zong-Hong Zhu

  • Department of Astronomy, Beijing Normal University, Beijing 100875, China

  • *Email address: hongsheng@bnu.edu.cn
  • Email address: zhuzh@bnu.edu.cn

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Issue

Vol. 73, Iss. 4 — 15 February 2006

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