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佐藤・廣島研 素粒子・宇宙物理研究室

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概要

In this talk we discuss a model in which neutrino masses are generated via radiative correction realized by interactions associated with leptoquarks.

We first review phenomenology regarding leptoquarks. Then we discuss the model structure applying modular flavor symmetry.

Focusing on neutrino mass matrix, results of numerical analysis of the model are shown where we obtain some predictions about neutrino observables.