Are neutrino oscillation mixings linked to the smallness of solar neutrino scale?
Observed reactor and atmospheric neutrino oscillation mixing values appear to be related to the neutrino scale ratio p ∆m2 sol/∆2 ATM in a way that suggest that the neutrino mass matrix can be expanded as a power series by using this ratio as the smallness parameter. This approach provides a simple and natural way to expose the inner hierarchies among neutrino mass terms, which amounts to also explain the solar oscillation mixing as well as solar oscillation scale. We explore a class of mass matrix textures that realize this scenario, for both normal and inverted neutrino mass hierarchies, as well as CP violation and their stability under renormalization scaling.
Authors
- Abdel Pérez-Lorenzana (ORCID: https://orcid.org/0000-0001-9442-3538)
- Eduardo Becerra-García (ORCID: https://orcid.org/0000-0002-8474-8053)
Institutions
- Instituto Politécnico Nacional (MX)
- Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional (MX)
Publication Details
- Journal
- Revista Mexicana de Física
- Published
- 2024-09-01
- DOI
- https://doi.org/10.31349/revmexfis.70.050801
- Citations
- 1
- Primary Topic
- Neutrino Physics Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00