Pilgrim Dark Energy Bianchi Type-I f(T) Gravity Model

Authors

DOI:

https://doi.org/10.26565/2312-4334-2024-3-09

Keywords:

Pilgrim dark energy, Dark matter, f(T) Gravity, Bianchi type-I space-time, Cosmology

Abstract

In this work, we have analyzed Bianchi type-I space-time (spatially homogeneous and anisotropic), using an interacting two fluid - dark matter (DM) and Pilgrim dark energy (PDE) in the framework of f(T) gravity by taking into consideration the infrared (IR) cut-off as a candidate of Hubble’s horizon L=1/H. We have also performed the state-finder diagnostics and in addition, energy conditions are discussed to verify accelerating expansion of the universe.

Author Biography

  • Kishor S. Wankhade, P. G. Department of Mathematics, Yashwantrao Chavan Arts and Science Mahavidyalaya, Mangrulpirб Dist. Washim, (M.S.) India

    Associate Professor and Head, P. G. Department of Mathematics

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Published

2024-09-02

Issue

No. 3 (2024): East European Journal of Physics

Section

Original Papers

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How to Cite

Pilgrim Dark Energy Bianchi Type-I f(T) Gravity Model. (2024). East European Journal of Physics, 3, 93-102. https://doi.org/10.26565/2312-4334-2024-3-09

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