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

Abstract 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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Main Authors: Zhi-zhong Xing, Shun Zhou, Ye-Ling Zhou
Format: Article
Language:English
Published: SpringerOpen 2018-05-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP05(2018)015
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spelling doaj-5699515f2cdf4b948457e5ad93920cff2020-11-25T01:11:32ZengSpringerOpenJournal of High Energy Physics1029-84792018-05-012018512310.1007/JHEP05(2018)015Renormalization-group equations of neutrino masses and flavor mixing parameters in matterZhi-zhong Xing0Shun Zhou1Ye-Ling Zhou2Institute of High Energy Physics, Chinese Academy of SciencesInstitute of High Energy Physics, Chinese Academy of SciencesInstitute for Particle Physics Phenomenology, Department of Physics, Durham UniversityAbstract 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≡22GFNeE $$ a\equiv 2\sqrt{2}\kern0.5em {G}_{\mathrm{F}}{N}_eE $$ 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 $$ {\tilde{m}}_i $$ (for i = 1, 2, 3). Given the standard parametrization of V , the RGEs for θ˜12,θ˜13,θ˜23,δ˜ $$ \left\{{\tilde{\theta}}_{12},\kern0.5em {\tilde{\theta}}_{13},\kern0.5em {\tilde{\theta}}_{23},\kern0.5em \tilde{\delta}\right\} $$ 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.http://link.springer.com/article/10.1007/JHEP05(2018)015Neutrino PhysicsRenormalization Group
collection DOAJ
language English
format Article
sources DOAJ
author Zhi-zhong Xing
Shun Zhou
Ye-Ling Zhou
spellingShingle Zhi-zhong Xing
Shun Zhou
Ye-Ling Zhou
Renormalization-group equations of neutrino masses and flavor mixing parameters in matter
Journal of High Energy Physics
Neutrino Physics
Renormalization Group
author_facet Zhi-zhong Xing
Shun Zhou
Ye-Ling Zhou
author_sort Zhi-zhong Xing
title Renormalization-group equations of neutrino masses and flavor mixing parameters in matter
title_short Renormalization-group equations of neutrino masses and flavor mixing parameters in matter
title_full Renormalization-group equations of neutrino masses and flavor mixing parameters in matter
title_fullStr Renormalization-group equations of neutrino masses and flavor mixing parameters in matter
title_full_unstemmed Renormalization-group equations of neutrino masses and flavor mixing parameters in matter
title_sort renormalization-group equations of neutrino masses and flavor mixing parameters in matter
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-05-01
description Abstract 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≡22GFNeE $$ a\equiv 2\sqrt{2}\kern0.5em {G}_{\mathrm{F}}{N}_eE $$ 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 $$ {\tilde{m}}_i $$ (for i = 1, 2, 3). Given the standard parametrization of V , the RGEs for θ˜12,θ˜13,θ˜23,δ˜ $$ \left\{{\tilde{\theta}}_{12},\kern0.5em {\tilde{\theta}}_{13},\kern0.5em {\tilde{\theta}}_{23},\kern0.5em \tilde{\delta}\right\} $$ 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.
topic Neutrino Physics
Renormalization Group
url http://link.springer.com/article/10.1007/JHEP05(2018)015
work_keys_str_mv AT zhizhongxing renormalizationgroupequationsofneutrinomassesandflavormixingparametersinmatter
AT shunzhou renormalizationgroupequationsofneutrinomassesandflavormixingparametersinmatter
AT yelingzhou renormalizationgroupequationsofneutrinomassesandflavormixingparametersinmatter
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