2021
DOI: 10.48550/arxiv.2108.04066
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Exploring Neutrino Masses and Mixing in the Seesaw Model with ${L_e-L_j}$ Gauged Symmetry

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“…Literature survey shows there are many flavor symmetries either discrete A 4 [23][24][25], S 3 [26][27][28][29], S 4 [30][31][32] etc. or continuous U (1) B−L [33][34][35][36][37], U (1) H [38][39][40], U (1) Le−Lτ [41,42] etc., which can generate the tiny neutrino masses and also accommodate the observed neutrino oscillation data with the help of some additional scalars and perturbation (wherever required). As aforesaid, inclusion of flavons affects the neatness of the model and the predictability of the model is hampered because of the higher dimensional operators.…”
Section: Introductionmentioning
confidence: 99%
“…Literature survey shows there are many flavor symmetries either discrete A 4 [23][24][25], S 3 [26][27][28][29], S 4 [30][31][32] etc. or continuous U (1) B−L [33][34][35][36][37], U (1) H [38][39][40], U (1) Le−Lτ [41,42] etc., which can generate the tiny neutrino masses and also accommodate the observed neutrino oscillation data with the help of some additional scalars and perturbation (wherever required). As aforesaid, inclusion of flavons affects the neatness of the model and the predictability of the model is hampered because of the higher dimensional operators.…”
Section: Introductionmentioning
confidence: 99%
“…It is interesting to notice that many non-abelian discrete symmetries i.e., S 3 [28][29][30][31], A 4 [32][33][34][35], S 4 [36][37][38] etc. and continuous symmetries like U (1) B−L [39][40][41][42][43][44][45], U (1) Le−Lµ [46][47][48][49], U (1) H [50][51][52][53] etc. come to our rescue to develop the model and generate neutrino mass matrix which gives results in-accordance with experimental data.…”
Section: Introductionmentioning
confidence: 99%