A dynamical system representation of generalized Rastall gravity
Hamid Shabani, Hooman Moradpour, Amir Hadi Ziaie

TL;DR
This paper analyzes a modified gravity model called generalized Rastall gravity using dynamical systems, showing it can produce a realistic cosmic evolution sequence and account for the Universe's accelerated expansion.
Contribution
It introduces a dynamical system framework for generalized Rastall gravity and demonstrates its viability in explaining cosmic acceleration and evolution.
Findings
Stable critical point for late-time acceleration.
Sequence from radiation to dark energy domination.
Consistency with observational data on spatial curvature.
Abstract
In this work we study the phase-space analysis of generalized Rastall gravity (GRG) which has recently been introduced as a modification to the original version of Rastall gravity (RG). In GRG, the coupling parameter assumes a dynamical feature and may play the role of dark energy (DE) which is responsible for the present accelerating expansion of the Universe. Our investigation shows that such a modification of General Relativity (GR) admits a stable critical point corresponding to the late time accelerated expansion of the Universe. Assuming both dark matter (DM) and an ultra-relativistic perfect fluid (radiation) as the cosmic ingredients, we find that the underlying model presents a viable sequence of cosmic evolution, beginning from radiation dominated era passing then through DM domination and finally reaches the late time DE dominated era. Moreover, taking into account the…
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