Leptogenesis
Sacha Davidson, Enrico Nardi, Yosef Nir
TL;DR
Leptogenesis connects neutrino mass generation to the cosmological baryon asymmetry by invoking the out-of-equilibrium decays of heavy sterile neutrinos that generate a lepton asymmetry, subsequently converted into a baryon asymmetry by sphalerons. The review clarifies the seesaw parameterizations, CP-violating sources, and the dynamical evolution via Boltzmann equations, while detailing finite-temperature effects, spectator processes, and crucial flavour dynamics that can dramatically alter outcomes. It shows that flavour, thermal corrections, and resonant or nonstandard scenarios can ease lower bounds on $M_1$ and open lower reheating temperatures in some models, though universal bounds persist in others. The work systematically catalogs the methods and limitations, highlighting how leptogenesis remains a compelling, testable framework within extensions of the Standard Model, and outlining the phenomenological implications for neutrino physics and cosmology.
Abstract
Leptogenesis is a class of scenarios where the baryon asymmetry of the Universe is produced from a lepton asymmetry generated in the decays of a heavy sterile neutrino. We explain the motivation for leptogenesis. We review the basic mechanism, and describe subclasses of models. We then focus on recent developments in the understanding of leptogenesis: finite temperature effects, spectator processes, and in particular the significance of flavor physics.
