中文

How to Test Stringy Dark Energy?

天体物理学 2009-11-07 v2 广义相对论与量子宇宙学 高能物理 - 唯象学 高能物理 - 理论

摘要

It is suggested, by using a covariant lagrangian formalism to estimate the equation of state w=p/ρw = p/\rho, that stringy dark energy predicts w<1w < -1, a negative pressure larger in magnitude than that for a cosmological constant or quintessence. This would lead to a later transition from decelerating to accelerating cosmological expansion; w=4/3w = - 4/3 is briefly considered as one illustrative example.

关键词

引用

@article{arxiv.astro-ph/0209037,
  title  = {How to Test Stringy Dark Energy?},
  author = {P. H. Frampton},
  journal= {arXiv preprint arXiv:astro-ph/0209037},
  year   = {2009}
}

备注

4 pages LaTeX. v2. Typos corrected