Thermodynamic parametrization of dark energy
  We propose a model-independent parametrization of dark energy motivated by
thermodynamics. To this aim, we consider Pad\'e polynomials to reconstruct the
form of deceleration parameter adequate to describe different epochs of cosmic
history and divergence-free in the far future. The proposed scenario also
fulfills the demand of structure formation and contains the $\Lambda$CDM model
as a limiting case. Thus, a numerical analysis at both background and
perturbation levels is performed through the Markov Chain Monte Carlo method in
view of the most recent cosmic data. We then use the observational constraints
to explore the features of dark energy evolution and compare our findings with
the predictions of the standard cosmological model.
