Littlest Modular Seesaw
Littlest Modular Seesaw
We present the first complete model of the Littlest Modular Seesaw, based on two right-handed neutrinos, within the framework of multiple modular symmetries, justifying the use of multiple moduli fields which take their values at 3 specific stabilizers of $\Gamma_4 \simeq S_4$, including a new phenomenological possibility. Using a semi-analytical approach, we perform a $\chi^2$ analysis of each case and show that good agreement with neutrino oscillation data is obtained, including predictive relations between the leptonic mixing angles and the ratio of light neutrino masses, which non-trivially agree with the experimental values. It is noteworthy that in this very predictive setup, the models fit the global fits of the experimental data remarkably well, both with and without the Super-Kamiokande atmospheric data, for both choices of stabilizers. By extending the model to include a weighton and the double cover group $\Gamma'_4 \simeq S'_4$, we are able to also account for the hierarchy of the charged leptons using modular symmetries, without altering the neutrino predictions.
hep-ph
Varzielas, Ivo de Medeiros
9e2b1443-1449-4687-8d03-2f67275730c0
King, Steve F.
f8c616b7-0336-4046-a943-700af83a1538
Levy, Miguel
972c27c0-44a5-4e33-8111-354f2860df82
Varzielas, Ivo de Medeiros
9e2b1443-1449-4687-8d03-2f67275730c0
King, Steve F.
f8c616b7-0336-4046-a943-700af83a1538
Levy, Miguel
972c27c0-44a5-4e33-8111-354f2860df82
[Unknown type: UNSPECIFIED]
Abstract
We present the first complete model of the Littlest Modular Seesaw, based on two right-handed neutrinos, within the framework of multiple modular symmetries, justifying the use of multiple moduli fields which take their values at 3 specific stabilizers of $\Gamma_4 \simeq S_4$, including a new phenomenological possibility. Using a semi-analytical approach, we perform a $\chi^2$ analysis of each case and show that good agreement with neutrino oscillation data is obtained, including predictive relations between the leptonic mixing angles and the ratio of light neutrino masses, which non-trivially agree with the experimental values. It is noteworthy that in this very predictive setup, the models fit the global fits of the experimental data remarkably well, both with and without the Super-Kamiokande atmospheric data, for both choices of stabilizers. By extending the model to include a weighton and the double cover group $\Gamma'_4 \simeq S'_4$, we are able to also account for the hierarchy of the charged leptons using modular symmetries, without altering the neutrino predictions.
Text
2211.00654v1
- Author's Original
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Accepted/In Press date: 1 November 2022
Additional Information:
16 pages, 2 Figures
Keywords:
hep-ph
Identifiers
Local EPrints ID: 472311
URI: http://eprints.soton.ac.uk/id/eprint/472311
PURE UUID: b4220d3b-5e40-484a-9673-ae51c244428d
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Date deposited: 30 Nov 2022 18:13
Last modified: 16 Mar 2024 23:05
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Contributors
Author:
Ivo de Medeiros Varzielas
Author:
Miguel Levy
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