Dark energy from cosmological fluids obeying a Shan-Chen nonideal equation of state

We consider a Friedmann-Robertson-Walker universe with a fluid source obeying a non-ideal equation of state with \lq\lq asymptotic freedom," namely ideal gas behavior (pressure changes directly proportional to density changes) both at low and high density regimes, following a fluid dynamical model due to Shan and Chen. It is shown that, starting from an ordinary energy density component, such fluids naturally evolve towards a universe with a substantial \lq\lq dark energy" component at the present time, with no need of invoking any cosmological constant. Moreover, we introduce a quantitative indicator of darkness abundance, which provides a consistent picture of the actual matter-energy content of the universe.