Phase space analysis of cosmological models on $f(R,G,T)$ gravity
Elangbam Chingkheinganba Meetei, S. Surendra Singh

TL;DR
This paper develops a dynamical system approach to analyze cosmological models within $f(R,G,T)$ gravity, demonstrating compatibility with observations and the $ ext{Lambda}$CDM model through stability analysis and data fitting.
Contribution
It introduces a new dynamical system formulation for $f(R,G,T)$ gravity and analyzes its solutions, stability, and observational consistency, which is novel in this modified gravity context.
Findings
Universe is currently dark energy dominated.
Cosmic acceleration with $q=-0.5$ and $ ext{w}=-0.66$ indicating Quintessence.
Model aligns with $ ext{Lambda}$CDM} based on observational data.
Abstract
In the present article, we developed a dynamical system in the context of modified gravity, where , and are Ricci scalar, Gauss-Bonnet term and energy-momentum tensor respectively. Development of the dynamical system is done by first defining 9 dimensionless variables and formulate a ordinary differential equations by taking derivative of the variables with respect to logarithmic time , where is the scale factor. This formulation is applied to the model , and its solutions and their corresponding stabilities are analysed in details. From the plot of density parameters vs , we conclude that our Universe is currently dominated by dark energy, which is compatible with current observation. Taking , cosmic parameters such as deceleration parameter , equation of state …
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Taxonomy
TopicsCosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics
