  We consider the FLRW universe in a loop quantum cosmological model filled
with the radiation, baryonic matter (with negligible pressure), dark energy and
dark matter. The dark matter sector is supposed to be of Bose-Einstein
condensate type. The Bose-Einstein condensation process in a cosmological
context by supposing it as an approximate first order phase transition, has
been already studied in the literature. Here, we study the evolution of the
physical quantities related to the early universe description such as the
energy density, temperature and scale factor of the universe, before, during
and after the condensation process. We also consider in detail the evolution
era of the universe in a mixed normal-condensate dark matter phase. The
behavior and time evolution of the condensate dark matter fraction is also
analyzed.
