Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matter

Abstract Neutrino oscillations in matter can be fully described by six effective parameters, namely, three neutrino mixing angles θ ˜ 12 θ ˜ 13 θ ˜ 23 $$ \left\{{\tilde{\theta}}_{12},{\tilde{\theta}}_{13},{\tilde{\theta}}_{23}\right\} $$ , one Dirac-type CP-violating phase δ ˜ $$ \tilde{\delta} $$ ,...

Full description

Bibliographic Details
Main Authors: Xin Wang, Shun Zhou
Format: Article
Language:English
Published: SpringerOpen 2019-05-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP05(2019)035
_version_ 1818109284985077760
author Xin Wang
Shun Zhou
author_facet Xin Wang
Shun Zhou
author_sort Xin Wang
collection DOAJ
description Abstract Neutrino oscillations in matter can be fully described by six effective parameters, namely, three neutrino mixing angles θ ˜ 12 θ ˜ 13 θ ˜ 23 $$ \left\{{\tilde{\theta}}_{12},{\tilde{\theta}}_{13},{\tilde{\theta}}_{23}\right\} $$ , one Dirac-type CP-violating phase δ ˜ $$ \tilde{\delta} $$ , and two neutrino mass-squared differences Δ ˜ 21 ≡ m ˜ 2 2 − m ˜ 1 2 $$ {\tilde{\Delta}}_{21}\equiv {\tilde{m}}_2^2-{\tilde{m}}_1^2 $$ and Δ ˜ 21 ≡ m ˜ 3 2 − m ˜ 1 2 $$ {\tilde{\Delta}}_{21}\equiv {\tilde{m}}_3^2-{\tilde{m}}_1^2 $$ . Recently, a complete set of differential equations for these effective parameters have been derived to characterize their evolution with respect to the ordinary matter term a ≡ 2 2 G F N e E $$ a\equiv 2\sqrt{2}{G}_{\mathrm{F}}{N}_eE $$ , in analogy with the renormalization-group equations (RGEs) for running parameters. Via series expansion in terms of the small ratio α c ≡ Δ21/Δc with Δc ≡ Δ31 cos2 θ12+Δ32 sin2 θ 12, we obtain approximate analytical solutions to the RGEs of the effective neutrino parameters and make several interesting observations. First, at the leading order, θ ˜ 12 $$ {\tilde{\theta}}_{12} $$ and θ ˜ 13 $$ {\tilde{\theta}}_{13} $$ are given by the simple formulas in the two-flavor mixing limit, while θ ˜ 23 ≈ θ 23 $$ {\tilde{\theta}}_{23}\approx {\theta}_{23} $$ and δ ˜ ≈ δ $$ \tilde{\delta}\approx \delta $$ are not changed by matter effects. Second, the ratio of the matter-corrected Jarlskog invariant J ˜ $$ \tilde{\mathcal{J}} $$ to its counterpart in vacuum J $$ \mathcal{J} $$ approximates to J ˜ / J ≈ 1 / C ^ 12 C ^ 13 $$ \tilde{\mathcal{J}}/\mathcal{J}\approx 1/\left({\widehat{C}}_{12}{\widehat{C}}_{13}\right) $$ , where C ^ 12 ≡ 1 − 2 A ∗ cos 2 θ 12 + A ∗ 2 $$ {\widehat{C}}_{12}\equiv \sqrt{1-2{A}_{\ast } \cos 2{\theta}_{12}+{A}_{{}^{\ast}}^2} $$ with A ∗ ≡ a/Δ21 and C ^ 13 ≡ 1 − 2 A c cos 2 θ 13 + A c 2 $$ {\widehat{C}}_{13}\equiv \sqrt{1-2{A}_c \cos 2{\theta}_{13}+{A}_c^2} $$ with Ac ≡ a/Δc have been defined. Finally, after taking higher-order corrections into account, we find compact and simple expressions of all the effective parameters, which turn out to be in perfect agreement with the exact numerical results.
first_indexed 2024-12-11T02:28:49Z
format Article
id doaj.art-28d07e70de224993bcd63c439ee78e16
institution Directory Open Access Journal
issn 1029-8479
language English
last_indexed 2024-12-11T02:28:49Z
publishDate 2019-05-01
publisher SpringerOpen
record_format Article
series Journal of High Energy Physics
spelling doaj.art-28d07e70de224993bcd63c439ee78e162022-12-22T01:23:52ZengSpringerOpenJournal of High Energy Physics1029-84792019-05-012019512010.1007/JHEP05(2019)035Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matterXin Wang0Shun Zhou1Theoretical Physics Division, Institute of High Energy PhysicsTheoretical Physics Division, Institute of High Energy PhysicsAbstract Neutrino oscillations in matter can be fully described by six effective parameters, namely, three neutrino mixing angles θ ˜ 12 θ ˜ 13 θ ˜ 23 $$ \left\{{\tilde{\theta}}_{12},{\tilde{\theta}}_{13},{\tilde{\theta}}_{23}\right\} $$ , one Dirac-type CP-violating phase δ ˜ $$ \tilde{\delta} $$ , and two neutrino mass-squared differences Δ ˜ 21 ≡ m ˜ 2 2 − m ˜ 1 2 $$ {\tilde{\Delta}}_{21}\equiv {\tilde{m}}_2^2-{\tilde{m}}_1^2 $$ and Δ ˜ 21 ≡ m ˜ 3 2 − m ˜ 1 2 $$ {\tilde{\Delta}}_{21}\equiv {\tilde{m}}_3^2-{\tilde{m}}_1^2 $$ . Recently, a complete set of differential equations for these effective parameters have been derived to characterize their evolution with respect to the ordinary matter term a ≡ 2 2 G F N e E $$ a\equiv 2\sqrt{2}{G}_{\mathrm{F}}{N}_eE $$ , in analogy with the renormalization-group equations (RGEs) for running parameters. Via series expansion in terms of the small ratio α c ≡ Δ21/Δc with Δc ≡ Δ31 cos2 θ12+Δ32 sin2 θ 12, we obtain approximate analytical solutions to the RGEs of the effective neutrino parameters and make several interesting observations. First, at the leading order, θ ˜ 12 $$ {\tilde{\theta}}_{12} $$ and θ ˜ 13 $$ {\tilde{\theta}}_{13} $$ are given by the simple formulas in the two-flavor mixing limit, while θ ˜ 23 ≈ θ 23 $$ {\tilde{\theta}}_{23}\approx {\theta}_{23} $$ and δ ˜ ≈ δ $$ \tilde{\delta}\approx \delta $$ are not changed by matter effects. Second, the ratio of the matter-corrected Jarlskog invariant J ˜ $$ \tilde{\mathcal{J}} $$ to its counterpart in vacuum J $$ \mathcal{J} $$ approximates to J ˜ / J ≈ 1 / C ^ 12 C ^ 13 $$ \tilde{\mathcal{J}}/\mathcal{J}\approx 1/\left({\widehat{C}}_{12}{\widehat{C}}_{13}\right) $$ , where C ^ 12 ≡ 1 − 2 A ∗ cos 2 θ 12 + A ∗ 2 $$ {\widehat{C}}_{12}\equiv \sqrt{1-2{A}_{\ast } \cos 2{\theta}_{12}+{A}_{{}^{\ast}}^2} $$ with A ∗ ≡ a/Δ21 and C ^ 13 ≡ 1 − 2 A c cos 2 θ 13 + A c 2 $$ {\widehat{C}}_{13}\equiv \sqrt{1-2{A}_c \cos 2{\theta}_{13}+{A}_c^2} $$ with Ac ≡ a/Δc have been defined. Finally, after taking higher-order corrections into account, we find compact and simple expressions of all the effective parameters, which turn out to be in perfect agreement with the exact numerical results.http://link.springer.com/article/10.1007/JHEP05(2019)035Neutrino PhysicsRenormalization Group
spellingShingle Xin Wang
Shun Zhou
Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matter
Journal of High Energy Physics
Neutrino Physics
Renormalization Group
title Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matter
title_full Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matter
title_fullStr Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matter
title_full_unstemmed Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matter
title_short Analytical solutions to renormalization-group equations of effective neutrino masses and mixing parameters in matter
title_sort analytical solutions to renormalization group equations of effective neutrino masses and mixing parameters in matter
topic Neutrino Physics
Renormalization Group
url http://link.springer.com/article/10.1007/JHEP05(2019)035
work_keys_str_mv AT xinwang analyticalsolutionstorenormalizationgroupequationsofeffectiveneutrinomassesandmixingparametersinmatter
AT shunzhou analyticalsolutionstorenormalizationgroupequationsofeffectiveneutrinomassesandmixingparametersinmatter