Non minimally coupled condensate cosmologies: matching observational
  data with phase space
  We compare theoretical predictions with observations for a class of
cosmological models in which the dark energy component is modeled as a
fermionic condensate, non-minimally coupled with the gravitational field and
characterized by some specific self-interaction potentials. Our analysis is
based on the Markov Chain Monte Carlo Method (MCMC) and employs different data
sets. It turns out that with an appropriate choice of parameters our models are
fully compatible with several observed data. We combine these parameter values
with phase space analysis to deduce the features of the entire cosmic history
of the considered models.
