[PDF] Top 20 Interacting dark fluids in bianchi type-i universe with variable deceleration parameter

... the universe has been well established through numerous and complementary cosmological ...of type Ia supernovae (SNIa) (Riess et ...currently universe is ...flat universe is dominated by an ... See full document

... of Bianchi type-V universe and con- jointly discovered that dark energy dominates the universe at the present ...accelerating dark energy model and explored some new exact ... See full document

... Bianchi type-I and V universes with wet dark ...the Bianchi type-VIo universe with matter term with dark energy treated as a Dark Fluid satisfying the ... See full document

... paper, Bianchi type- VIo cosmological model with Wet Dark Fluid (WDF) in f(R,T) gravity , where R is the Ricci scalar and T the trace of stress energy-momentum tensor, in the context of late time ... See full document

... LRS Bianchi type-II universe filled with minimally interacting dark matter and homographic dark ...holographic dark energy in the evolution of the universe. The ... See full document

... However, this restriction on the displacement field to be constant is only for convenience and there is no prior reason for it. Many authors studied the cosmological models with constant and time dependent displacement ... See full document

... the deceleration parameter ...and deceleration parameter q play an important role in describing the nature of evolution of the ...the universe to- day while the latter one characterizes ... See full document

... wet dark fluid. In this paper we study the Bianchi type- III and Kantowski-Sachs Universes with matter term with dark energy treated as a Dark Fluid satisfying the Equation of state ... See full document

... (LRS) Bianchi type - I cosmological model universe interacting with perfect fluid in the context of Lyra ...constant deceleration parameter models of the universe ... See full document

... holographic dark energy model in Brans – Dicke ...studied interacting holographic dark energy models in Brans-Dicke (1961) theory of ...of interacting holographic dark energy ... See full document

... anisotropy parameter shows that at time tends to infinity the anisotropy parameter tends to zero that is the universe tends to ...The deceleration parameter for this model is q   1 ... See full document

... of Bianchi types-I & V models in f ( R , T ) by using the assumption of constant deceleration parameter and variation of law of Hubble ...LRS Bianchi type-II universe ... See full document

... non-flat Bianchi type- II cosmological model in General Relativity in the presence of two minimally interacting fluids; a perfect fluid as the matter fluid and a hypothetical anisotropic fluid ... See full document

... anisotropic Bianchi type-V dark energy models by considering constant deceleration ...EoS parameter  is considered as a constant by Kujat et ...used dark energy models with time ... See full document

... the universe, many authors have used CDP to obtain cosmological models in the context of dark energy (DE) in general relativity and some other modified theories of gravitation such as f(R) theory within the ... See full document

... holographic dark energy and each one of phantom, tachyon, chaplygin gas and generalized chaplygin gas in FRW universe have been investigated by Setare [36] [37] [38] ...of interacting holographic ... See full document

... fluid type by assuming an equation of state linking the pressure p and energy density in order to build an analytical methodsnear the ...with variable equation of state, which essentially deals with the ... See full document

... expansion of the universe, assuming the time dependent average scale factor . As a consequence, we have found time dependent deceleration parameter q(t). Also, for a metric which is homogeneous ... See full document

... f R T = + R µ T . The dynamical parameters are calculated and analyzed with a new mathematical formalism in power law cosmology and hybrid scale factor cosmology. We have shown that there exist various values for inputs ... See full document

... the universe. It explained that the universe may have started from an initial singularity (an extremely hot dense phase generally refer to as the Planck ... See full document