Evolution of a Simple Inhomogeneous Anisotropic Cosmological Model with Diffusion

Abstract

We investigate a simple inhomogeneous anisotropic cosmology (plane symmetric $G_2$ model) filled with a tilted perfect fluid undergoing velocity diffusion on a scalar field. Considered are two types of fluid: dust and radiation. We solve the system of Einstein field equations and diffusion equations numerically and demonstrate how the universe evolves towards its future asymptotic state. Also, typical time scales of characteristic processes are determined. The obtained results for dust- and radiation-filled cosmologies are compared to each other and to those in the diffusionless case, giving a hint on which effects can be the result of including diffusion in more complicated models. For example, diffusion causes the accelerated expansion stage to arrive at later times.

17 pages, 6 figures

References in corpus (2)

• Relativistic diffusion
• Late-time behaviour of the tilted Bianchi type VIh models

Cited by in corpus (4)

• Dynamics of the diffusive DM-DE interaction--dynamical system approach
• Dynamics of Robertson-Walker spacetimes with diffusion
• Inhomogeneous and anisotropic Universe and apparent acceleration
• The late-time behaviour of tilted Bianchi type VIII universes in presence of diffusion