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- W2010338431 abstract "The lepton asymmetry that could be generated in the early universe through oscillations of active to sterile neutrinos is calculated (almost) analytically for small mixing angles, sin2θ<10−2. It is shown that for a mass squared difference, δm2=−1 eV2 it may rise at most by six orders of magnitude from the initial “normal” value ∼10−10, as the back-reaction from the refraction index terminates this rise while the asymmetry is still small. Only for very large mass differences, |δm2|∼109 eV2, the lepton asymmetry could reach a significant magnitude exceeding 0.1." @default.
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- W2010338431 title "Neutrino oscillations in the early universe: how can large lepton asymmetry be generated?" @default.
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- W2010338431 doi "https://doi.org/10.1016/s0927-6505(00)00111-0" @default.
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