中文

Acceleration at z>1?

天体物理学 2009-11-07 v3 广义相对论与量子宇宙学 高能物理 - 唯象学

摘要

Most models of dark energy predict the beginning of the accelerated epoch at z <= 1. However, there are no observational or theoretical evidences in favor of such a recent start of the cosmic acceleration. In fact, a model of dark energy coupled to dark matter is explicitely constructed that a) is accelerated even at high z; b) allows structure formation during acceleration; and c) is consistent with the type Ia supernovae Hubble diagram, including the farthest known supernova SN1997ff at z~1.7 . It is shown that the accelerated epoch in this model could have started as early as z~5.

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引用

@article{arxiv.astro-ph/0209494,
  title  = {Acceleration at z>1?},
  author = {Luca Amendola},
  journal= {arXiv preprint arXiv:astro-ph/0209494},
  year   = {2009}
}

备注

11 pages, submitted to MNRAS. v2: added a ref. v3: another ref