Effective description of dark matter as a viscous fluid
  Treating dark matter at large scales as an effectively viscous fluid provides
an improved framework for the calculation of the density and velocity power
spectra compared to the standard assumption of an ideal pressureless fluid. We
discuss how this framework can be made concrete through an appropriate
coarse-graining procedure. We also review results that demonstrate that it
improves the convergence of cosmological perturbation theory.
