Constraints and cosmography of $\Lambda$CDM in presence of viscosity

Abstract

In this work, we study two scenarios of the Universe filled by a perfect fluid following the traditional dark energy and a viscous fluid as dark matter. In this sense, we explore the simplest case for the viscosity in the Eckart formalism, a constant, and then, a polynomial function of the redshift. We constrain the phase-space of the model parameters by performing a Bayesian analysis based on Markov Chain Monte Carlo method and using the latest data of the Hubble parameter (OHD), Type Ia Supernovae (SNIa) and Strong Lensing Systems. The first two samples cover the region $0.01<z<2.36$. Based on AIC, we find equally support of these viscous models over Lambda-Cold Dark Matter (LCDM) taking into account OHD or SNIa. On the other hand, we reconstruct the cosmographic parameters ($q,j,s,l$) and find good agreement to LCDM within up to $3\sigma$ CL. Additionally, we find that the cosmographic parameters and the acceleration-deceleration transition are sensible to the parameters related to the viscosity coefficient, making of the viscosity an interesting physical mechanism to modified them.

Accepted for publication in EPJC

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• The Nature of Dark Energy and Constraints on Its Hypothetical Constituents from Force Measurements
• A non-singular early-time viscous cosmological model
• Viscous fluid dynamics with decaying vacuum energy density
• Observational constraints and dynamical analysis of Kaniadakis horizon-entropy cosmology
• Kaniadakis holographic dark energy: observational constraints and global dynamics
• Testing a nonlinear solution of the Israel-Stewart theory