  We study the quark hadron phase transition in the framework of massive
gravity. We show that the modification of the FRW cosmological equations leads
to the quark hadron phase transition in the early massive Universe. Using
numerical analysis, we consider that a phase transition based on the chiral
symmetry breaking after the electroweak transition, occurred at approximately
$10 \mu$ seconds after the Big Bang to convert a plasma of free quarks and
gluons into hadrons.
