Dark Energy Universe in Bianchi Type-I Cosmological Model

  • Priyanka Garg


 In the present work, there is a trend to modify the earlier models (supporting the constant rate of expansion), by assuming the time-dependent average scale factor a(t) = [(c1t + c2)(m + 2)]1/3 .  Here, we have also revisited the investigation of new holographic dark energy. The Saez-Ballester field equations are solved under certain assumptions and found a power law of expansion.  Our model and its current range for DE, ω  (EoS) parameter is observed to be in great concurrence from the observations. Also, for the model, Some physical and geometric aspects of the DE model are also highlighted.

How to Cite
Priyanka Garg. (2020). Dark Energy Universe in Bianchi Type-I Cosmological Model. International Journal of Advanced Science and Technology, 29(05), 9037-9045. Retrieved from http://sersc.org/journals/index.php/IJAST/article/view/18749