Are neutrino oscillation mixings linked to the smallness of solar neutrino scale?

Authors

  • Eduardo Becerra-García Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional
  • Abdel Pérez-Lorenzana Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional

DOI:

https://doi.org/10.31349/RevMexFis.70.050801

Keywords:

Neutrino mass matrix; reactor

Abstract

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.

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Published

2024-09-01

How to Cite

[1]
E. Becerra-García and A. Pérez-Lorenzana, “Are neutrino oscillation mixings linked to the smallness of solar neutrino scale?”, Rev. Mex. Fís., vol. 70, no. 5 Sep-Oct, pp. 050801 1–, Sep. 2024.