$\Lambda$CDM-type cosmological model and observational constraints

Abstract

In the present work, we have searched the existence of $\Lambda$CDM-type cosmological model in anisotropic Heckmann-Schucking space-time. The matter source that is responsible for the present acceleration of the universe consist of cosmic fluid with $p=\omega \rho$, where $\omega$ is the equation of state parameter. The Einstein's field equations have been solved explicitly under some specific choice of parameters that isotropizes the model under consideration. It has been found that the derived model is in good agreement with recent SN Ia observations. Some physical aspects of the model has been discussed in detail.

11 pages, 3 groups of plots, 2 tables

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• Two Fluid Scenario in Bianchi Type-I Universe
• Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
• Anisotropic String Cosmological Models in Heckmann-Suchuking Space-Time
• Bianchi type-I Dust Filled Accelerating Brans- Dicke Cosmology
• $\Lambda$-CDM type Heckmann - Suchuking model and union 2.1 compilation
• An exact solution of the observable universe in Bianchi V space-time