论文标题

中微子振荡是否与太阳中微子量表的较小相关?

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

论文作者

Becerra-García, Eduardo, Pérez-Lorenzana, Abdel

论文摘要

观察到的反应器和大气中微子振荡混合值似乎与中微子尺度比率$ \ sqrt {Δm^2_ {sol}/δ{sol}/δ^2_ {atm}} $,以表明可以通过以下比率来将中微子质量矩阵作为电力序列扩展为中性中微子质量矩阵。这种方法提供了一种简单而自然的方式来揭示中微子质量术语之间的内部层次结构,这还等同于解释太阳振荡混合以及太阳能振荡量表。我们探索了一类质量基质纹理,这些质地意识到这种情况,无论是正常和倒立的中微子质量层次结构,以及CP违规及其在重新归一化缩放下的稳定性及其稳定性。

Observed reactor and atmospheric neutrino oscillation mixing values appear to be related to the neutrino scale ratio $\sqrt{Δm^2_{sol}/Δ^2_{ATM}}$ 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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