On the Stability of Einstein Universe in f(R,T,R_{μν}T^{μν}) Gravity

Abstract

This paper investigates the existence and stability of Einstein universe in the context of $f(R,T,Q)$ gravity, where $Q=R_{\mu \nu }{T}^{\mu \nu }$. Considering linear homogeneous perturbations around scale factor and energy density, we formulate static as well as perturbed field equations. We parameterize the stability regions corresponding to conserved as well as non-conserved energy-momentum tensor using linear equation of state parameter for particular models of this gravity. The graphical analysis concludes that for a suitable choice of parameters, the stable regions of the Einstein universe are obtained.

18 pages, 4 figures

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Cited by in corpus (4)

• Coincident f(Q) gravity: black holes, regular black holes and black bounces
• Stability of the Closed Einstein Universe in Energy-Momentum Squared Gravity
• Gödel-type solutions in $f(R,T,R_{\mu \nu }{T}^{\mu \nu }$) gravity
• Late time dynamics of $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ gravity