Non-Static Plane Symmetric Cosmological Model with Magnetized Anisotropic Dark Energy by Hybrid Expansion Law in Gravity
- Department of Mathematics, Phulsing Naik Mahavidyalaya, Pusad-445216 (India).
- Department of Mathematics, G. S. G. Mahavidyalaya, Umarkhed-445206 (India).
- Department of Mathematics, Dr. B. N. College of Engg. & Tech., Yavatmal-44500 (India).
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In the presence of magnetized anisotropic Dark Energy (DE) fluid, some features of non-static plane symmetric universe with anisotropic Equation of State (EoS) parameter are investigated in gravity. We choose Hybrid Expansion Law (HEL) which exhibits a transition of the universe from decelerating phase to the present accelerating phase, to obtain the determinate solution. We found that the EoS parameter for the dark energy is time-dependent and its existing range for derived models is in good agreement with data obtained from recent theoretical observations [1-4]. The physical and geometric aspects of the universe are also discussed in detail.
[S.R.Bhoyar, V.R.Chirde, S.H. Shekh (2015); Non-Static Plane Symmetric Cosmological Model with Magnetized Anisotropic Dark Energy by Hybrid Expansion Law in Gravity Int. J. of Adv. Res. 3 (Sep). 492-500] (ISSN 2320-5407). www.journalijar.com
