  We consider baryogenesis in quantum fluctuation modified gravity. We explore
three forms (two are newly proposed here) of baryogenesis interaction and
discuss the effect of these interaction terms on the baryon-to-entropy ratio
during the radiation era of the expanding universe. We constrain the model
parameters with the current observational data, implying that this modified
gravity is capable to address the issue of baryon asymmetry in a successful
manner.
