Renormalization-group equations of neutrino masses and flavor mixing parameters in matter

A bstract We borrow the general idea of renormalization-group equations (RGEs) to understand how neutrino masses and flavor mixing parameters evolve when neutrinos propagate in a medium, highlighting a meaningful possibility that the genuine flavor quantities in vacuum can be extrapolated from their...

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Published inThe journal of high energy physics Vol. 2018; no. 5; pp. 1 - 23
Main Authors Xing, Zhi-zhong, Zhou, Shun, Zhou, Ye-Ling
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 01.05.2018
Springer Nature B.V
SpringerOpen
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Summary:A bstract We borrow the general idea of renormalization-group equations (RGEs) to understand how neutrino masses and flavor mixing parameters evolve when neutrinos propagate in a medium, highlighting a meaningful possibility that the genuine flavor quantities in vacuum can be extrapolated from their matter-corrected counterparts to be measured in some realistic neutrino oscillation experiments. Taking the matter parameter a ≡ 2 2 G F N e E to be an arbitrary scale-like variable with N e being the net electron number density and E being the neutrino beam energy, we derive a complete set of differential equations for the effective neutrino mixing matrix V and the effective neutrino masses m ˜ i (for i = 1 , 2 , 3). Given the standard parametrization of V , the RGEs for θ ˜ 12 , θ ˜ 13 , θ ˜ 23 , δ ˜ in matter are formulated for the first time. We demonstrate some useful differential invariants which retain the same form from vacuum to matter, including the well-known Naumov and Toshev relations. The RGEs of the partial μ - τ asymmetries, the off-diagonal asymmetries and the sides of unitarity triangles of V are also obtained as a by-product.
ISSN:1029-8479
1029-8479
DOI:10.1007/JHEP05(2018)015