FRW cosmology with varying cubic deceleration parameter
Leishingam Kumrah, S. Surendra Singh, L. Anjana Devi, Md Khurshid, Alam

TL;DR
This paper introduces a new third-degree law for the deceleration parameter in FRW cosmology, deriving solutions that describe a cyclic universe with Big Bang and Big Rip singularities, and analyzes its physical and dynamical properties.
Contribution
A novel third-degree varying deceleration parameter law is proposed, leading to new cosmological solutions with cyclic behavior and singularities.
Findings
Universe exhibits Big Bang and Big Rip singularities.
Model shows cyclic evolution with phases of expansion and contraction.
Graphical analysis confirms the behavior of physical parameters.
Abstract
In this work a new law of varying deceleration parameter of third degree have been proposed. The solutions of the modified field equations have been derived under the newly proposed law of the deceleration parameter. Model exhibits the Big-bang singularity at cosmic time () and shows Big Rip at () then it re-enter the phase of initial singularity at and ends its cyclic behavior at . The evolution of the physical and dynamical parameters of the Universe have been studied and the graphical representation has also been shown. Further diagnostic parameter and the energy conditions have also been studied together with their graphical representations.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Computational Physics and Python Applications
