Quantum mechanics of baryogenesis
arXiv:hep-ph/0004145 · doi:10.1016/S0370-2693(00)00573-6
Abstract
The cosmological baryon asymmetry can be explained as remnant of heavy Majorana neutrino decays in the early universe. We study this out-of-equilibrium process by means of Kadanoff-Baym equations which are solved in a perturbative expansion. To leading order the problem is reduced to solving a set of Boltzmann equations for distribution functions.
12 pages, 2 figures, typos corrected. To be published in Physics Letters
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