Scotogenic majorana neutrino masses in a predictive orbifold theory of flavour
arXiv:2110.06810 · doi:10.1103/PhysRevD.105.055030
Abstract
The use of extra space-time dimensions provides a promising approach to the flavour problem. The chosen compactification of a 6-dimensional orbifold implies a remnant family symmetry . This makes interesting predictions for quark and lepton masses, for neutrino oscillations and neutrinoless double beta decay, providing also a very good global description of all flavour observables. Due to an auxiliary symmetry, we implement a scotogenic Majorana neutrino mass generation mechanism with a viable WIMP dark matter candidate.
17 pages, 4 figures, 2 tables. v2: matches published version
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- The symmetry approach to quark and lepton masses and mixing
- Flavour and dark matter in a scoto/type-II seesaw model
- Absolute neutrino mass scale and dark matter stability from flavour symmetry
- Discrete symmetries and Efficient Counting of Operators
- Quark-lepton mass relations from modular flavor symmetry