  Dark energy is an elusive concept, which has been introduced two decades ago
in order to make the acceleration of the universe a comprehensible phenomenon.
However, the nature of this energy is far from being understood, both from a
fundamental as well as an observational way. In this work we study cosmological
consequences of the existence of particles (which we called ``ewkons'' in a
previous work) which are quasi distinguishable, obey unorthodox statistics, and
have an equation of state similar to many existent dark energy candidates
(including negative relation between pressure and energy density). We find an
effective scalar field description of this ewkon fluid, and obtain cosmological
solutions for the dark energy dominated epoch. This can be considered as a
one-parameter class of dark energy models.
