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The Standard Model accompanied with two right-handed neutrinos with themasses below the weak scale can explain the observed baryon asymmetry of theUniverse. Moreover, this model is at least partially testable in theforthcoming experiments such as NA62, SHiP, and MATHUSLA. The remarkableprogress in understanding of various rates entering the kinetic equationsdescribing the asymmetry generation along with considerable improvements of thenumerical procedures allow us to perform a comprehensive analysis of theparameter space of the model. We find that the region of parameters leading tothe successful baryogenesis is notably larger than it was previously obtained.Our results are presented in a way that they can be readily used for studies ofsensitivity of various experiments searching for the right-handed neutrinosresponsible for the baryon asymmetry of the Universe. We also present adetailed comparison with the studies by other groups.

Parameter space of baryogenesis in the $\nu$MSM