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| DOI | 10.1007/JHEP05(2021)215 | ||||
| Año | 2021 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
We propose a 3+1 Higgs Doublet Model based on the ∆(27) family symmetry supplemented by several auxiliary cyclic symmetries leading to viable Yukawa textures for the Standard Model fermions, consistent with the observed pattern of fermion masses and mixings. The charged fermion mass hierarchy and the quark mixing pattern is generated by the spontaneous breaking of the discrete symmetries due to flavons that act as Froggatt-Nielsen fields. The tiny neutrino masses arise from a radiative seesaw mechanism at one loop level, thanks to a preserved Z2(1) discrete symmetry, which also leads to stable scalar and fermionic dark matter candidates. The leptonic sector features the predictive cobimaximal mixing pattern, consistent with the experimental data from neutrino oscillations. For the scenario of normal neutrino mass hierarchy, the model predicts an effective Majorana neutrino mass parameter in the range 3 meV ≲ mββ ≲ 18 meV, which is within the declared range of sensitivity of modern experiments. The model predicts Flavour Changing Neutral Currents which constrain the model, for instance, μ→e nuclear conversion processes and Kaon mixing are found to be within the reach of the forthcoming experiments.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | CARCAMO-HERNANDEZ, ANTONIO ENRIQUE | Hombre |
Universidad Técnica Federico Santa María - Chile
Centro Científico Tecnológico de Valparaíso - Chile |
| 2 | de Medeiros Varzielas, I. | Hombre |
Instituto Superior Técnico - Portugal
Univ Lisbon - Portugal |
| 3 | López-Ibáñez, M. L. | - |
Institute of Theoretical Physics Chinese Academy of Sciences - China
CASSACA - China |
| 4 | Melis, Aurora | Mujer |
National Institute of Chemical Physics and Biophysics, Tallinn - Estonia
NICPB - Estonia |
| Fuente |
|---|
| China Postdoctoral Science Foundation |
| Fundacao para a Ciencia e a Tecnologia (FCT) |
| National Science Center, Poland, through the HARMONIA project |
| ANID-Chile FONDECYT |
| FCT through QREN |
| EU through the European Regional Development Fund CoE program "The Dark Side of the Universe" |
| FCT through EU |
| FCT through COMPETE |
| Estonian Research Council grants |
| FCT through POCTI (FEDER) |
| Agradecimiento |
|---|
| The authors thank Avelino Vicente for very useful discussions. A.E.C.H. is supported by ANID-Chile FONDECYT 1210378. IdMV acknowledges funding from Fundacao para a Ciencia e a Tecnologia (FCT) through the contract IF/00816/2015 and was supported in part by the National Science Center, Poland, through the HARMONIA project under contract UMO-2015/18/M/ST2/00518, and by FCT through projects CFTP-FCT Unit 777 (UID/FIS/00777/2019), PTDC/FIS-PAR/29436/2017, CERN/FIS-PAR/0004/2019 and CERN/FIS-PAR/0008/2019 which are partially funded through POCTI (FEDER), COMPETE, QREN and EU. MLLI acknowledges support from the China Postdoctoral Science Foundation No.2020M670475. AM acknowledges support by the Estonian Research Council grants PRG803 and MOBTT86, and by the EU through the European Regional Development Fund CoE program TK133 "The Dark Side of the Universe". |