Kadanoff-Baym approach to the thermal resonant leptogenesis

preprint2014arXivOpen access

Abstract

Using the non-equilibrium Green function method (Kadanoff-Baym equations) in the expanding universe, we investigate evolution of the lepton number asymmetry when the right-handed (RH) neutrinos have almost degenerate masses ∣Mi2−Mj2∣≪Mi2|M_i^2-M_j^2| \ll M_i^2. The resonantly enhanced CPCP-violating parameter εi\varepsilon_i associated with the decay of the RH neutrino NiN_i is obtained. It is proportional to an enhancement factor (Mi2−Mj2)MiΓj/((Mi2−Mj2)2+Rij2)(M_i^2-M_j^2) M_i Γ_j/ ((M_i^2-M_j^2)^2 +R_{ij}^2) with the regulator Rij=MiΓi+MjΓjR_{ij}=M_i Γ_i+M_j Γ_j. The result is consistent with the previous result obtained by Garny et al., in a constant background with an out-of-equilibrium initial state. We discuss the origin of such a regulator, and why it is not like Rij=MiΓi−MjΓjR_{ij}=M_i Γ_i-M_j Γ_j.

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