Three-loop induced neutrino mass model in a non-invertible symmetry
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arXiv
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| Format: | Preprint |
| Publié: |
2025
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| _version_ | 1866916855723065344 |
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| author | Okada, Hiroshi Shigekami, Yoshihiro |
| author_facet | Okada, Hiroshi Shigekami, Yoshihiro |
| contents | We propose a new type of radiatively induced neutrino masses at three-loop level based on the Ma model, introducing a non-invertible symmetry in the class under a ${\mathbb Z_2}$ gauging of ${\mathbb Z_6}$ symmetry and adding three isospin doublet vector-like fermions $L'$ and singlet boson $S_0$. Under this symmetry, the Yukawa interactions directly related to the neutrino masses are not allowed at tree-level. However it is allowed at one-loop level due to $L'$ and $S_0$ as well as $η$, which is no longer invariant under this symmetry. Therefore, the symmetry is dynamically broken. Intriguingly, $η$ plays important roles in contributing to both the radiative matrices $y^η$ and $m_ν$. After constructing our model, we show some numerical analyses to satisfy the lepton flavor violations, muon anomalous magnetic dipole moment, and a boson dark matter candidate $S_0$ or $η_R$ for the cases of normal hierarchy and inverted hierarchy. Then, we demonstrate allowed space for our input parameters. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_16198 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Three-loop induced neutrino mass model in a non-invertible symmetry Okada, Hiroshi Shigekami, Yoshihiro High Energy Physics - Phenomenology We propose a new type of radiatively induced neutrino masses at three-loop level based on the Ma model, introducing a non-invertible symmetry in the class under a ${\mathbb Z_2}$ gauging of ${\mathbb Z_6}$ symmetry and adding three isospin doublet vector-like fermions $L'$ and singlet boson $S_0$. Under this symmetry, the Yukawa interactions directly related to the neutrino masses are not allowed at tree-level. However it is allowed at one-loop level due to $L'$ and $S_0$ as well as $η$, which is no longer invariant under this symmetry. Therefore, the symmetry is dynamically broken. Intriguingly, $η$ plays important roles in contributing to both the radiative matrices $y^η$ and $m_ν$. After constructing our model, we show some numerical analyses to satisfy the lepton flavor violations, muon anomalous magnetic dipole moment, and a boson dark matter candidate $S_0$ or $η_R$ for the cases of normal hierarchy and inverted hierarchy. Then, we demonstrate allowed space for our input parameters. |
| title | Three-loop induced neutrino mass model in a non-invertible symmetry |
| topic | High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2507.16198 |