Bianchi type-V modified holographic Ricci dark energy models in Saez-Ballester theory of gravitation

We have investigated Bianchi type-V universe filled with matter and modified holographic Ricci dark energy in a scalar-tensor theory proposed by Saez-Ballester (Phys. Lett. A., 113, 467, 1986). To get a determinate solution, we have used (i) hybrid expansion law (Akarsu et al. JCAP, 01, 022, 2014), (ii) varying deceleration parameter (Mishra et al. Int. J. Theor. Phys. 52, 2546, 2013) and (iii) linearly varying deceleration parameter (Akarsu and Dereli, Int. J. Theor. Phys. 51, 612, 2012). The various physical and geometrical aspects of the models are also discussed.The accepted manuscript in pdf format is listed with the files at the bottom of this page. The presentation of the authors' names and (or) special characters in the title of the manuscript may differ slightly between what is listed on this page and what is listed in the pdf file of the accepted manuscript; that in the pdf file of the accepted manuscript is what was submitted by the author