Examining the Viscous Ricci Dark Energy Cosmological Model in General Theory of Gravitation

  • T. Chinnappalanaidu Department of Mathematics, Vignan’s Institute of Information Technology(Autonomous), Visakhapatnam, India https://orcid.org/0000-0001-6902-2820
  • M. Vijaya Santhi Department of Applied Mathematics, College of Science and Technology, Andhra University, Visakhapatnam, India https://orcid.org/0000-0002-0050-3033
  • N. Sri Lakshmi Sudha Rani Department of Applied Mathematics, College of Science and Technology, Andhra University, Visakhapatnam, India https://orcid.org/0009-0009-9593-954X
Keywords: Dark energy, Viscous Ricci dark energy, Marder type metric, General relativity

Abstract

This study focuses on dynamically exploring Marder-type spacetime containing viscous Ricci dark energy within the framework of general relativity theory. To find a solution of the field equations, we use the relation between metric potentials and the average scale factor a(t)=(sinhβ1t)1/β2, this leads to a seamless transition of the Universe from its initial decelerating phase to the current accelerating phase. Here, we have obtained the cosmological parameters and ωde-ω'de plane for the derived model. Also, dynamical features of the derived cosmological model are analyzed through diagrams.

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Published
2024-09-02
Cited
How to Cite
Chinnappalanaidu, T., Santhi, M. V., & Rani, N. S. L. S. (2024). Examining the Viscous Ricci Dark Energy Cosmological Model in General Theory of Gravitation. East European Journal of Physics, (3), 71-82. https://doi.org/10.26565/2312-4334-2024-3-07