LambdaCDM Model with dissipative nonextensive dark matter
Viscous Cosmology, nonextensivity, NexDC Correspondence
Many models in cosmology typically assume the standard bulk viscosity. On this thesis, we study an alternative interpretation for the origin of the bulk viscosity. Using nonadditive statistics proposed by Tsallis, we propose a bulk viscosity component that can only exist by a nonextensive effect through the nonextensive/dissipative correspondence (NexDC). We consider the LambdaCDM model for a flat universe with a dissipative nonextensive viscous dark matter component, following the Eckart theory of bulk viscosity, without any perturbative approach. In order to analyse cosmological constraints, we use one of the most recent observations of Type Ia Supernova, baryon acoustic oscillations and cosmic microwave background data. It's shown that only exists viscous effect in 2 sigma confidence level scenarios.