Protecting the primordial baryon asymmetry in the seesaw model compatible with WMAP and KamLAND

Abstract

We require that the primordial baryon asymmetry is not washed out in the seesaw model compatible with the recent results of WMAP and the neutrino oscillation experiments including the first results of KamLAND. We find that only the case of the normal neutrino mass hierarchy with an approximate $L_e$-symmetry satisfies the requirement. We further derive, depending on the signs of neutrino mass eigenvalues, three types of neutrino mass matrixes, where the values of each element are rather precisely fixed.

21pages; added references

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Cited by in corpus (3)

• Dark Energy from Mass Varying Neutrinos
• Protecting the primordial baryon asymmetry in the $SU(2{)}_L$ triplet Higgs model compatible with KamLAND and WMAP
• Time variation of particle and anti-particle asymmetry in an expanding universe