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Splitting of Three Nearly Mass-Degenerate Neutrinos

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arxiv hep-ph/9812344 v2 pith:ZMPARMHM submitted 1998-12-12 hep-ph

Ernest Ma (UC Riverside) This is my paper · ORCID
classification hep-ph
keywords neutrinoneutrinososcillationsthreeamountassumingatmosphericbroken
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abstract

Assuming the canonical seesaw mechanism together with an SO(3) family symmetry for leptons, broken only by the charged-lepton masses, I show that the three neutrinos of Majorana mass $m_0$ are split radiatively in two loops by a maximum finite calculable amount of order $10^{-9} m_0$. This is very suitable for dark matter and vacuum solar neutrino oscillations. I also discuss how atmospheric neutrino oscillations can be incorporated.

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  1. Complete Two-loop Renormalization Group Equation of the Weinberg Operator

    hep-ph 2024-11 accept novelty 7.0 of 10

    The full two-loop renormalization group equation of the dimension-5 Weinberg operator in the Standard Model is derived, completing the two-loop RGE program of SMEFT up to dimension 5.

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