Neutrino transition magnetic moment in the $U(1)_X$SSM
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arXiv
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| Autori principali: | , , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866909689110855680 |
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| author | Ruan, Long Zhao, Shu-Min Liu, Ming-Yue Han, Xing-Yu Wang, Xi Dong, Xing-Xing |
| author_facet | Ruan, Long Zhao, Shu-Min Liu, Ming-Yue Han, Xing-Yu Wang, Xi Dong, Xing-Xing |
| contents | This paper investigates the neutrino transition magnetic moment in the $U(1)_X$SSM. $U(1)_X$SSM is the $U(1)$ extension of Minimal Supersymmetric Standard Model (MSSM) and its local gauge group is extended to $SU(3)_C\times SU(2)_L \times U(1)_Y\times U(1)_X$. To obtain this model, three singlet new Higgs superfields and right-handed neutrinos are added to the MSSM, which can explain the results of neutrino oscillation experiments. The neutrino transition magnetic moment is induced by electroweak radiative corrections. By applying effective Lagrangian method and on-shell scheme, we study the associated Feynman diagrams and the transition magnetic moment of neutrinos in the model. We fit experimental data for neutrino mass variances and mixing angle. Based on the range of data selection, the influences of different sensitive parameters on the results are analysed. The numerical analysis shows that many parameters have an effect on the neutrino transition moment, such as $g_X$, $M_2$, $λ_H$ and $g_{YX}$. For our numerical results, the order of magnitude of $μ_{ij}^M/μ_B$ is around $10^{-20}$ $\sim$ $10^{-19}$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_05741 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Neutrino transition magnetic moment in the $U(1)_X$SSM Ruan, Long Zhao, Shu-Min Liu, Ming-Yue Han, Xing-Yu Wang, Xi Dong, Xing-Xing High Energy Physics - Phenomenology This paper investigates the neutrino transition magnetic moment in the $U(1)_X$SSM. $U(1)_X$SSM is the $U(1)$ extension of Minimal Supersymmetric Standard Model (MSSM) and its local gauge group is extended to $SU(3)_C\times SU(2)_L \times U(1)_Y\times U(1)_X$. To obtain this model, three singlet new Higgs superfields and right-handed neutrinos are added to the MSSM, which can explain the results of neutrino oscillation experiments. The neutrino transition magnetic moment is induced by electroweak radiative corrections. By applying effective Lagrangian method and on-shell scheme, we study the associated Feynman diagrams and the transition magnetic moment of neutrinos in the model. We fit experimental data for neutrino mass variances and mixing angle. Based on the range of data selection, the influences of different sensitive parameters on the results are analysed. The numerical analysis shows that many parameters have an effect on the neutrino transition moment, such as $g_X$, $M_2$, $λ_H$ and $g_{YX}$. For our numerical results, the order of magnitude of $μ_{ij}^M/μ_B$ is around $10^{-20}$ $\sim$ $10^{-19}$. |
| title | Neutrino transition magnetic moment in the $U(1)_X$SSM |
| topic | High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2407.05741 |