Sphaleron-induced baryon-number nonconservation and a constraint on Majorana neutrino masses

Physics

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Scientific paper

We point out that the baryon-number asymmetry in the Universe is erased by the sphaleron effect just below the electroweak phase transition irrespective of the primordial baryon- and lepton-number asymmetry, if there exists a Majorana-type interaction. The requirement to avoid this happening leads to the condition that mν (Majorana) <50 keV for all species of neutrinos, regardless of whether or not neutrinos are stable.

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