Phantom Cosmic Dynamics: Tracking Attractor and Cosmic Doomsday
天体物理学
2009-11-10 v3 广义相对论与量子宇宙学
高能物理 - 理论
摘要
We study the dynamics of phantom model and give the conditions for potentials to admit tracking attractor, de Sitter attractor and big rip attractor. Especially, we show that phantom models with exponential and inverse power law potentials do not admit the tracking attractor solution. The "tachyonic" stability of the system at/near the attractors as well as the quantum stabiltiy have been studied.
引用
@article{arxiv.astro-ph/0309746,
title = {Phantom Cosmic Dynamics: Tracking Attractor and Cosmic Doomsday},
author = {Jian-gang Hao and Xin-zhou Li},
journal= {arXiv preprint arXiv:astro-ph/0309746},
year = {2009}
}
备注
7 pages, 6 figures; Replaced with the version to be published in Physical Review D. A discussion concerning the quantum stability added