Phase space analysis in $f(R,L_{m})$ gravity with scalar field
Y. Kalpana Devi, Rahul Bhagat, B. Mishra

TL;DR
This paper explores the cosmological dynamics of $f(R, \\mathcal{L}_m)$ gravity with scalar fields, revealing stable late-time accelerated expansion and matter-dominated phases through dynamical system analysis.
Contribution
It introduces a detailed dynamical system analysis of $f(R, \\mathcal{L}_m)$ gravity with scalar fields, including stability of critical points and late-time acceleration solutions.
Findings
Existence of matter-dominated and accelerated phases.
Stable late-time de Sitter-like attractors.
Transition from decelerated to accelerated expansion.
Abstract
In this work, we investigate the cosmological dynamics of the gravity framework with a particular focus on the contributions of the scalar field. Considering a functional form that includes linear and exponential dependence on the matter Lagrangian, we perform a detailed dynamical system analysis by introducing appropriate dimensionless variables and constructing the corresponding autonomous system. The critical points are obtained and analyzed, and due to their non-hyperbolic nature, center manifold theory is employed to determine their stability. The analysis reveals the existence of matter-dominated and accelerated phases of the Universe, along with a transition from a decelerated to an accelerated expansion. We further extend the model by incorporating a minimally coupled generalized scalar field with a kinetic term and an exponential self-interacting…
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