$$A_4$$ A4 realization of linear seesaw and neutrino phenomenology

Abstract Motivated by the crucial role played by the discrete flavor symmetry groups in explaining the observed neutrino oscillation data, we consider the $$A_4$$ A4 realization of linear seesaw by extending the standard model (SM) particle content with two types of right-handed (RH) neutrinos along...

Full description

Bibliographic Details
Main Authors: M. Sruthilaya, Rukmani Mohanta, Sudhanwa Patra
Format: Article
Language:English
Published: SpringerOpen 2018-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-6181-6
id doaj-7e1c3a07ad8f428798a3944985f9f014
record_format Article
spelling doaj-7e1c3a07ad8f428798a3944985f9f0142020-11-24T21:36:01ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-09-0178911510.1140/epjc/s10052-018-6181-6$$A_4$$ A4 realization of linear seesaw and neutrino phenomenologyM. Sruthilaya0Rukmani Mohanta1Sudhanwa Patra2School of Physics, University of HyderabadSchool of Physics, University of HyderabadIndian Institute of Technology Bhilai, GEC CampusAbstract Motivated by the crucial role played by the discrete flavor symmetry groups in explaining the observed neutrino oscillation data, we consider the $$A_4$$ A4 realization of linear seesaw by extending the standard model (SM) particle content with two types of right-handed (RH) neutrinos along with the flavon fields, and the SM symmetry with $$A_4\times Z_4\times Z_3$$ A4×Z4×Z3 and a global symmetry $$U(1)_X$$ U(1)X , which is broken explicitly by the Higgs potential. We scrutinize this model to see if it can explain the recent results from neutrino oscillation experiments, by searching for parameter space that can accommodate the observables such as the reactor mixing angle $$\theta _{13}$$ θ13 , the CP violating phase $$\delta _\text {CP}$$ δCP , sum of active neutrino masses $$\Sigma _{i} m_i$$ Σimi , solar and atmospheric mass-squared differences, and the lepton number violating parameter called the effective Majorana mass parameter, in line with recent experimental results. We also discuss the scope of this model to explain the baryon asymmetry of the Universe through leptogenesis. We also investigate the possibility of probing the non-unitarity effect in this scenario, but it is found to be rather small.http://link.springer.com/article/10.1140/epjc/s10052-018-6181-6
collection DOAJ
language English
format Article
sources DOAJ
author M. Sruthilaya
Rukmani Mohanta
Sudhanwa Patra
spellingShingle M. Sruthilaya
Rukmani Mohanta
Sudhanwa Patra
$$A_4$$ A4 realization of linear seesaw and neutrino phenomenology
European Physical Journal C: Particles and Fields
author_facet M. Sruthilaya
Rukmani Mohanta
Sudhanwa Patra
author_sort M. Sruthilaya
title $$A_4$$ A4 realization of linear seesaw and neutrino phenomenology
title_short $$A_4$$ A4 realization of linear seesaw and neutrino phenomenology
title_full $$A_4$$ A4 realization of linear seesaw and neutrino phenomenology
title_fullStr $$A_4$$ A4 realization of linear seesaw and neutrino phenomenology
title_full_unstemmed $$A_4$$ A4 realization of linear seesaw and neutrino phenomenology
title_sort $$a_4$$ a4 realization of linear seesaw and neutrino phenomenology
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2018-09-01
description Abstract Motivated by the crucial role played by the discrete flavor symmetry groups in explaining the observed neutrino oscillation data, we consider the $$A_4$$ A4 realization of linear seesaw by extending the standard model (SM) particle content with two types of right-handed (RH) neutrinos along with the flavon fields, and the SM symmetry with $$A_4\times Z_4\times Z_3$$ A4×Z4×Z3 and a global symmetry $$U(1)_X$$ U(1)X , which is broken explicitly by the Higgs potential. We scrutinize this model to see if it can explain the recent results from neutrino oscillation experiments, by searching for parameter space that can accommodate the observables such as the reactor mixing angle $$\theta _{13}$$ θ13 , the CP violating phase $$\delta _\text {CP}$$ δCP , sum of active neutrino masses $$\Sigma _{i} m_i$$ Σimi , solar and atmospheric mass-squared differences, and the lepton number violating parameter called the effective Majorana mass parameter, in line with recent experimental results. We also discuss the scope of this model to explain the baryon asymmetry of the Universe through leptogenesis. We also investigate the possibility of probing the non-unitarity effect in this scenario, but it is found to be rather small.
url http://link.springer.com/article/10.1140/epjc/s10052-018-6181-6
work_keys_str_mv AT msruthilaya a4a4realizationoflinearseesawandneutrinophenomenology
AT rukmanimohanta a4a4realizationoflinearseesawandneutrinophenomenology
AT sudhanwapatra a4a4realizationoflinearseesawandneutrinophenomenology
_version_ 1725942737725816832