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 in | The journal of high energy physics Vol. 2018; no. 5; pp. 1 - 23 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Berlin/Heidelberg
Springer Berlin Heidelberg
01.05.2018
Springer Nature B.V SpringerOpen |
Subjects | |
Online Access | Get full text |
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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. |
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ISSN: | 1029-8479 1029-8479 |
DOI: | 10.1007/JHEP05(2018)015 |