Anisotropic magnetized holographic Ricci dark energy cosmological models

In this paper, we have considered spatially homogeneous and anisotropic Bianchi type-III space-time filled with matter and anisotropic modified holographic Ricci dark energy in general relativity. We have solved the Einstein’s field equations using the following possibilities: (i) hybrid expansion law proposed by Akarsu et al. (JCAP, 01, 022, 2014)(ii) a varying deceleration parameter considered by Mishra et al. (Int. J. Theor. Phys. 52, 2546, 2013) and (iii) a linearly varying deceleration parameter given by Akarsu and Dereli (Int. J. Theor. Phys. 51, 612, 2012). We have presented the cosmological models in each of the above cases and studied their evolutions. We have also discussed physical and kinematical properties of the models.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