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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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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1725171122641567744 |