  In this work, we consider the gravitational baryogenesis in the framework of
non-minimal derivative coupling model. A mechanism to generate the baryon
asymmetry based on the coupling between the derivative of the Ricci scalar
curvature and the baryon current in context of non-minimal derivative coupling
model is investigated. We show that, in this model, the temperature increases
during the reheating periods to the end of reheating period or beginning of
radiation dominated era. Therefore the reheating temperature is larger then
decoupling temperature. It can be demonstrated that, the evaluation of baryon
asymmetry is not depends on coupling constant. In this model we can generate
baryon asymmetry at low and high reheating temperature, by considering the high
friction constraint.
