Fabris JC, de Oliveira PLC, Velten H. Constraints on unified models for dark matter and dark energy using H(z). European Physical Journal C. 2011;71(10): 1773.The differential age data of astrophysical objects that have evolved passively during the history of the universe (e. g. red galaxies) allows us to test theoretical cosmological models through the predicted Hubble function expressed in terms of the redshift z, H(z). We use the observational data for H(z) to test unified scenarios for dark matter and dark energy. Specifically, we focus our analysis on the Generalized Chaplygin Gas (GCG) and the viscous fluid (VF) models. For the GCG model, it is shown that the unified scenario for dark energy and dark matter requires some priors. For t...
In this work we explore an alternative phenomenological model to Chaplygin gas proposed by Hova et a...
AbstractWe constrain a unified dark matter (UDM) model from the latest observational data. This mode...
Unified Dark Matter models aim to describe thedynamical properties of Dark Matter and Dark Energyas ...
The differential age data of astrophysical objects that have evolved passively during the history of...
Velten H, Fabris JC, de Oliveira PLC. Constraints on unified models for dark matter and dark energy ...
In this paper, we use the latest observations of quasars covering the redshift range of $$0.04<z<5.1...
We investigate observational constraints on the generalized Chaplygin gas (GCG) model as the unifica...
Velten H, Schwarz D. Constraints on dissipative unified dark matter. Journal of Cosmology and Astrop...
In this paper, after reconstructing the redshift evolution of the Hubble function by adopting Gaussi...
We study the holographic and agegraphic dark energy models without interaction using the latest obse...
The modified Chaplygin gas could be considered to abide by the unified dark fluid model because the ...
Although various cosmological observations congruously suggest that our universe is dominated by tw...
So far large and different data sets revealed the accelerated expansion rate of the Universe, which ...
Although various cosmological observations congruously suggest that our universe is dominated by two...
We examine observational constraints on the generalized Chaplygin gas (GCG) model for dark energy fr...
In this work we explore an alternative phenomenological model to Chaplygin gas proposed by Hova et a...
AbstractWe constrain a unified dark matter (UDM) model from the latest observational data. This mode...
Unified Dark Matter models aim to describe thedynamical properties of Dark Matter and Dark Energyas ...
The differential age data of astrophysical objects that have evolved passively during the history of...
Velten H, Fabris JC, de Oliveira PLC. Constraints on unified models for dark matter and dark energy ...
In this paper, we use the latest observations of quasars covering the redshift range of $$0.04<z<5.1...
We investigate observational constraints on the generalized Chaplygin gas (GCG) model as the unifica...
Velten H, Schwarz D. Constraints on dissipative unified dark matter. Journal of Cosmology and Astrop...
In this paper, after reconstructing the redshift evolution of the Hubble function by adopting Gaussi...
We study the holographic and agegraphic dark energy models without interaction using the latest obse...
The modified Chaplygin gas could be considered to abide by the unified dark fluid model because the ...
Although various cosmological observations congruously suggest that our universe is dominated by tw...
So far large and different data sets revealed the accelerated expansion rate of the Universe, which ...
Although various cosmological observations congruously suggest that our universe is dominated by two...
We examine observational constraints on the generalized Chaplygin gas (GCG) model for dark energy fr...
In this work we explore an alternative phenomenological model to Chaplygin gas proposed by Hova et a...
AbstractWe constrain a unified dark matter (UDM) model from the latest observational data. This mode...
Unified Dark Matter models aim to describe thedynamical properties of Dark Matter and Dark Energyas ...