Panorama behaviors of Holographic Dark Energy models in f(R,T) gravity

2019/12/03 by A. Y. Shaikh, Shaikh, A. Y., K. S. Wankhade +1
Earth and Planetary Sciences · Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Physics (physics.gen-ph) #Geophysics and Gravity Measurements #physics.gen-ph

paper · pdf · doi:10.48550/arxiv.1912.08044

arxiv created 2019/12/03 · openalex publication_date 2019/12/03 · arxiv updated 2019/12/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Classes of solutions of field equations in gravity for a Bianchi sort I (Kasner form) space-time with matter and Holographic Dark Energy (HDE) is mentioned. Precise solutions of field equations are obtained with volumetrical power and exponential expansion laws .The physical and geometrical parameters of the models are mentioned well. The statefinder diagnostic pair and jerk parameter are analyzed to characterize utterly totally different phases of the universe.

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