Accelerating Anisotropic Cosmological Model Filled with Two Fluid and ∧
S. M. Borikar

S. M. Borikar, Department of Applied Mathematics, SIPNA College of Engineering and Technology, Amravati, India.
Manuscript received on February 06, 2020. | Revised Manuscript received on February 10, 2020. | Manuscript published on February 30, 2020. | PP: 1590-1592 | Volume-9 Issue-3, February, 2020. | Retrieval Number: C5664029320/2020©BEIESP | DOI: 10.35940/ijeat.C5664.029320
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© The Authors. Blue Eyes Intelligence Engineering and Sciences Publication (BEIESP). This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/)

Abstract: In this paper we have studied Kantowski-Sachs universe filled with perfect fluid and radiation with a cosmological constant. To get determinate solution, it is assumed that the scalar of expansion is proportional to shear scalar (    ) which leads to the relation between metric potentials n R= AS The cosmological parameters of models are also discussed.
Keywords: Perfect fluid, Radiation, cosmological constant, Kantowski-Sachs space-time.