Generalized Model of Interacting Dark Energy and Dark Matter : Phase Portrait Analysis of Evolving Universe
Giridhari Deogharia, Mayukh Bandyopadhyay, Ritabrata Biswas

TL;DR
This paper develops a three-fluid cosmological model with interacting dark energy and dark matter to explain the universe's accelerated expansion, analyzing stability and phase evolution through autonomous systems and phase portraits.
Contribution
It introduces a novel three-fluid interacting model with a specific interaction kernel and analyzes its stability, revealing conditions for late-time acceleration and dark energy dominance.
Findings
Identification of stable critical points representing dark energy dominated era
Graphical analysis showing late-time cosmic acceleration
No indication of future deceleration in the model
Abstract
Main aim of this work is to give a suitable explanation of present accelerating universe through an acceptable interactive dynamical cosmological model. A three-fluid cosmological model is introduced in the background of Friedmann-Lema\^itre-Robertson-Walker asymptotically flat spacetime. This model consists of interactive dark matter and dark energy with baryonic matter taken as perfect fluid satisfying barotropic equation of state. We consider dust as the candidate of dark matter. A scalar field represents dark energy with potential . Einstein's field equations are utilised to construct a three-dimensional interactive autonomous system by choosing suitable interaction between dark energy and dark matter. We take the interaction kernel as . In order to explain the stability of this system, we obtained some suitable critical points. We…
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