Bianchi V Brane-world Cosmology with a Generalized Chaplygin Gas

TL;DR

This paper explores exact solutions in Bianchi V brane-world cosmology with a generalized Chaplygin gas, analyzing dark energy and dark matter interactions and their effects on cosmic expansion and anisotropy.

Contribution

It provides new exact solutions for anisotropic brane cosmology incorporating a generalized Chaplygin gas, enhancing understanding of dark energy and dark matter interactions.

Findings

Behavior of expansion parameters analyzed

Anisotropy evolution studied

Dark energy and dark matter interactions modeled

Abstract

In the context of brane cosmology, we investigate exact solution of the gravitational field equations in the Randall-Sundrum model for an anisotropic brane with Bianchi V geometry, with a generalized Chaplygin gas, which plays the role of dark energy and interacts with dark matter particles. Also, the behavior of the observationally important parameters like expansion and anisotropy is examined.