The Grimus–Neufeld Model with FlexibleSUSY at One-Loop

The Grimus−Neufeld model can explain the smallness of measured neutrino masses by extending the Standard Model with a single heavy neutrino and a second Higgs doublet, using the seesaw mechanism and radiative mass generation. The Grimus−Lavoura approximation allows us to calculat...

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Main Authors: Simonas Draukšas, Vytautas Dūdėnas, Thomas Gajdosik, Andrius Juodagalvis, Paulius Juodsnukis, Darius Jurčiukonis
Format: Article
Language:English
Published: MDPI AG 2019-11-01
Series:Symmetry
Subjects:
Online Access:https://www.mdpi.com/2073-8994/11/11/1418
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spelling doaj-444abd1deb0f4a9fba96f938587cb4362020-11-25T02:21:19ZengMDPI AGSymmetry2073-89942019-11-011111141810.3390/sym11111418sym11111418The Grimus–Neufeld Model with FlexibleSUSY at One-LoopSimonas Draukšas0Vytautas Dūdėnas1Thomas Gajdosik2Andrius Juodagalvis3Paulius Juodsnukis4Darius Jurčiukonis5Institute of Theoretical Physics and Astronomy, Faculty of Physics, Vilnius University, Saulėtekio av. 3, 10257 Vilnius, LithuaniaInstitute of Theoretical Physics and Astronomy, Faculty of Physics, Vilnius University, Saulėtekio av. 3, 10257 Vilnius, LithuaniaInstitute of Theoretical Physics and Astronomy, Faculty of Physics, Vilnius University, Saulėtekio av. 3, 10257 Vilnius, LithuaniaInstitute of Theoretical Physics and Astronomy, Faculty of Physics, Vilnius University, Saulėtekio av. 3, 10257 Vilnius, LithuaniaInstitute of Theoretical Physics and Astronomy, Faculty of Physics, Vilnius University, Saulėtekio av. 3, 10257 Vilnius, LithuaniaInstitute of Theoretical Physics and Astronomy, Faculty of Physics, Vilnius University, Saulėtekio av. 3, 10257 Vilnius, LithuaniaThe Grimus−Neufeld model can explain the smallness of measured neutrino masses by extending the Standard Model with a single heavy neutrino and a second Higgs doublet, using the seesaw mechanism and radiative mass generation. The Grimus−Lavoura approximation allows us to calculate the light neutrino masses analytically. By inverting these analytic expressions, we determine the neutrino Yukawa couplings from the measured neutrino mass differences and the neutrino mixing matrix. Short-cutting the full renormalization of the model, we implement the Grimus−Neufeld model in the spectrum calculator FlexibleSUSY and check the consistency of the implementation. These checks hint that FlexibleSUSY is able to do the job of numerical renormalization in a restricted parameter space. As a summary, we also comment on further steps of the implementation and the use of FlexibleSUSY for the model.https://www.mdpi.com/2073-8994/11/11/1418neutrinosseesaw mechanismradiative massesspectrum calculator
collection DOAJ
language English
format Article
sources DOAJ
author Simonas Draukšas
Vytautas Dūdėnas
Thomas Gajdosik
Andrius Juodagalvis
Paulius Juodsnukis
Darius Jurčiukonis
spellingShingle Simonas Draukšas
Vytautas Dūdėnas
Thomas Gajdosik
Andrius Juodagalvis
Paulius Juodsnukis
Darius Jurčiukonis
The Grimus–Neufeld Model with FlexibleSUSY at One-Loop
Symmetry
neutrinos
seesaw mechanism
radiative masses
spectrum calculator
author_facet Simonas Draukšas
Vytautas Dūdėnas
Thomas Gajdosik
Andrius Juodagalvis
Paulius Juodsnukis
Darius Jurčiukonis
author_sort Simonas Draukšas
title The Grimus–Neufeld Model with FlexibleSUSY at One-Loop
title_short The Grimus–Neufeld Model with FlexibleSUSY at One-Loop
title_full The Grimus–Neufeld Model with FlexibleSUSY at One-Loop
title_fullStr The Grimus–Neufeld Model with FlexibleSUSY at One-Loop
title_full_unstemmed The Grimus–Neufeld Model with FlexibleSUSY at One-Loop
title_sort grimus–neufeld model with flexiblesusy at one-loop
publisher MDPI AG
series Symmetry
issn 2073-8994
publishDate 2019-11-01
description The Grimus−Neufeld model can explain the smallness of measured neutrino masses by extending the Standard Model with a single heavy neutrino and a second Higgs doublet, using the seesaw mechanism and radiative mass generation. The Grimus−Lavoura approximation allows us to calculate the light neutrino masses analytically. By inverting these analytic expressions, we determine the neutrino Yukawa couplings from the measured neutrino mass differences and the neutrino mixing matrix. Short-cutting the full renormalization of the model, we implement the Grimus−Neufeld model in the spectrum calculator FlexibleSUSY and check the consistency of the implementation. These checks hint that FlexibleSUSY is able to do the job of numerical renormalization in a restricted parameter space. As a summary, we also comment on further steps of the implementation and the use of FlexibleSUSY for the model.
topic neutrinos
seesaw mechanism
radiative masses
spectrum calculator
url https://www.mdpi.com/2073-8994/11/11/1418
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