http://arxiv.org/abs/1408.1101
In this letter we study the semi holographic model which corresponds to the radiative version of the model proposed by Zhang et al. (Phys. Lett. B 694 (2010), 177) and revisited by C\’ardenas et al. (Mon. Not. Roy. Astron. Soc. 438 (2014), 3603). This inclusion makes the model more realistic, so allows us to test it with current observational data and then answer if the inconsistency reported by C\’ardenas et al. is relaxed.
S. Campo, V. Cardenas, J. Magana, et. al.
Thu, 7 Aug 14
25/46
Comments: 14 pages, 6 figures. arXiv admin note: text overlap with arXiv:1306.6612
You must be logged in to post a comment.