| Issue |
EPJ Web Conf.
Volume 315, 2024
International Workshop on Future Linear Colliders (LCWS2024)
|
|
|---|---|---|
| Article Number | 01017 | |
| Number of page(s) | 5 | |
| Section | Physics | |
| DOI | https://doi.org/10.1051/epjconf/202431501017 | |
| Published online | 18 December 2024 | |
https://doi.org/10.1051/epjconf/202431501017
Testing the gauged U(1)B–L model for loop induced neutrino mass with dark matter*
Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
* OU-HET-1246
** speaker
Published online: 18 December 2024
We present a new viable benchmark scenario under the current experimental data for the model which can explain tiny mass of active neutrinos and dark matter, as a summary of Ref. [1]. Majorana masses of right-handed neutrinos are given by the spontaneous breaking of the U(1)B−L gauge symmetry above the electroweak scale, and tiny neutrino masses are radiatively induced by quantum effects of particles of the dark sector including dark matter candidates. We first show benchmark points which satisfy current experimental data, and then give comments on how this model can be tested at collider experiments.
© The Authors, published by EDP Sciences, 2024
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