Cosmological Models Coupled with Dark Matter in a Dissipative Universe

Abstract

We consider the cosmological system with two interacting fluids: dark energy and dark matter, in a homogeneous and isotropic universe with dissipation. The modified gravitational equation for dark matter is solved. The analytic representations for the Little Rip, the Pseudo Rip, and the bounce cosmology models with dissipation are obtained in terms of the thermodynamic parameters in the equation of state. We analyze the corrections in the energy density for dark matter, in view of the dissipative processes and the coupling with dark energy.

arXiv comment6 pages, no figures; to appear in Astrophysics and Space Science

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Cited by in corpus (9)

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• Testing the equation of state for viscous dark energy
• On structure formation from a small-scales-interacting dark sector
• Recent advances in cosmological singularities
• Dissipative Universe-Inflation with Soft Singularity
• Cosmological evolution of thermal relic particles in $f(R)$ gravity
• Viscous Accelerating Universe with Non-linear and Logarithmic Equation of State Fluid
• Little Rip, Pseudo Rip and bounce cosmology with generalized equation of state in non-standard backgrounds
• Non-linear Phenomenology of Disformally Coupled Quintessence