We use the dissipative-type theory (DTT) framework to solve for the evolution of conformal
fluids in Bjorken and Gubser flows from isotropic initial conditions. The results compare well …

We compute the dispersion relations for scalar, vector and tensor modes of a viscous
relativistic fluid, linearized around an equilibrium solution, for a divergence type theory …

We study the impact of the viscous effects of the primordial plasma on the evolution of the
primordial gravitational waves (pGW) spectrum from Inflation until today, considering a self …

A bstract In the Second Order Theories (SOT) of real relativistic fluids, the non-ideal
properties of the flows are described by a new set of dynamical tensor variables. In this work …

We consider the evolution of the gravitational wave spectrum for super-Hubble modes in
interaction with a relativistic fluid, which is regarded as an effective description of fluctuations …

We study the onset of vector instabilities in the post-inflationary epoch of the Universe as a
mechanism for primordial magnetic fields amplification. We assume the presence of a …

In this paper we address the derivation of causal relativistic hydrodynamics, formulated
within the framework of divergence type theories (DTTs), from kinetic theory for spinless …

Just as non-relativistic fluids, oftentimes we find relativistic fluids in situations where random
fluctuations cannot be ignored, with thermal and turbulent fluctuations being the most …

In the Second Order Theories (SOT) of real relativistic fluids, the non-ideal properties are
described by a new set of dynamical tensor variables. In this work we explore the non-linear …