Contraints on unified models for dark matter and dark energy using H(z)
  The differential age data of astrophysical objects that have evolved
passivelly during the history of the universe (e.g. red galaxies) allows 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 the VF model
we obtain estimations for the free parameters that may be compared with further
analysis mainly at perturbative level.
