Dynamics of Interacting Generalized Cosmic Chaplygin gas in Brane-world scenario

TL;DR

This paper investigates the dynamics of Generalized Cosmic Chaplygin Gas as dark energy in brane-world cosmologies, analyzing its role in cosmic acceleration, stability, and singularity avoidance through numerical and phase space methods.

Contribution

It introduces a detailed analysis of GCCG in DGP and RSII brane models, exploring interaction effects and stability, and assesses its viability for explaining late-time acceleration.

Findings

GCCG can drive late cosmic acceleration in RSII brane models.

Stable scaling solutions are obtained through numerical analysis.

Models are free from future singularities under studied conditions.

Abstract

In this work we explore the background dynamics when dark energy is coupled to dark matter with a suitable interaction in the universe described by brane cosmology. Here DGP and the RSII brane models have been considered separately. Dark energy in the form of Generalized Cosmic Chaplygin gas is considered. A suitable interaction between dark energy and dark matter is considered in order to at least alleviate (if not solve) the cosmic coincidence problem. The dynamical system of equations is solved numerically and a stable scaling solution is obtained. A significant attempt towards the solution of the cosmic coincidence problem is taken. The statefinder parameters are also calculated to classify the dark energy models. Graphs and phase diagrams are drawn to study the variations of these parameters. It is also seen that the background dynamics of Generalized Cosmic Chaplygin gas is consistent with the late cosmic acceleration, but not without satisfying certain conditions. It has been shown that the universe in both the models follows the power law form of expansion around the critical point, which is consistent with the known results. Future singularities were studied and our models were declared totally free from any types of such singularities. Finally, some cosmographic parameters were also briefly studied. Our investigation led to the fact that although GCCG with a far lesser negative pressure compared to other DE models, can overcome the relatively weaker gravity of RS II brane, with the help of the negative brane tension, yet for the DGP brane model with much higher gravitation, the incompetency of GCCG is exposed, and it cannot produce the accelerating scenario until it reaches the phantom era.