Thermodynamics of ghost dark energy in case of various nonlinear interactions
Institute for Physical Research, National Academy of Sciences, Ashtarak, Republic of Armenia
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Revised: 3 April 2016
Accepted: 24 April 2016
Published online: 27 May 2016
In this paper we discuss thermodynamics of interacting ghost dark energy models in a flat FRW universe. During the discussion our attention will be concentrated on nonlinear interactions of particular form. In the considered models dark matter is assumed to be a pressureless matter and allows to complete the darkness of the low-redshift universe. Ghost dark energy it is one of the models of dark energy among others with an explicitly given energy density as a function of the Hubble parameter of the universe. Our study aims to have a contribution towards recently suggested interacting ghost dark energy models.
© Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg, 2016