Comment on "A holographic model of dark energy and the thermodynamics of a nonflat accelerated expanding universe", by M.R. Setare and S. Shafei (JCAP 09 (2006) 011, arXiv:grqc/0606103)
Abstract
Authors of ref. [1], M.R. Setare and S. Shafei (JCAP 09 (2006) 011), studied the thermodynamics of a holographic dark energy model in a nonflat universe enclosed by the apparent horizon $R_A$ and the event horizon measured from the sphere of the horizon named $L$. In section 3 in ref. [1], Authors showed that for $R_A$ the generalized second law of thermodynamics is respected, while for $L$ it is satisfied for the special range of the deceleration parameter. Here we present that their calculations for $R_A$ should be revised. Also we show that their conclusion for $L$ is not true and the generalized second law is hold for the present time independently of the deceleration parameter. Also if we take into account the contribution of dark matter in the generalized second law which is absent in ref. [1], then the generalized second law for $L$ is violated for the present time.
 Publication:

arXiv eprints
 Pub Date:
 February 2010
 DOI:
 10.48550/arXiv.1002.0431
 arXiv:
 arXiv:1002.0431
 Bibcode:
 2010arXiv1002.0431K
 Keywords:

 Physics  General Physics;
 General Relativity and Quantum Cosmology
 EPrint:
 5 pages