Kento Asai (Institute for Cosmic Ray Research (ICRR), The University of Tokyo, Kashiwa, Chiba, 277–8582, Japan, Department of Physics, Faculty of Engineering Science, Yokohama National University, Yokohama, 240–8501, Japan); Sho Iwamoto (Institute for Theoretical Physics, ELTE Eötvös Loránd University, Budapest, H-1117, Hungary, Department of Physics, National Sun Yat-sen University, Kaohsiung, 804351, Taiwan, Center for Theoretical and Computational Physics, National Sun Yat-sen University, Kaohsiung, 804351, Taiwan); Maxim Perelstein (Department of Physics, LEPP, Cornell University, Ithaca, NY, 14853, USA); Yasuhito Sakaki (Radiation Science Center, High Energy Accelerator Research Organization (KEK), Ibaraki, 305–0801, Japan, The Graduate University for Advanced Studies (SOKENDAI), Hayama, 240–0193, Japan); Daiki Ueda (Center for High Energy Physics, Peking University, Beijing, 100871, China, Theory Center, High Energy Accelerator Research Organization (KEK), 1-1 Oho, Tsukuba, Ibaraki, 305-0801, Japan)

Published on:
16 February 2024
Created on:
17 February 2024
Publisher:
Springer
Published in:

Journal of High Energy Physics, Volume 2024 (2024) Issue 2Pages 1-35

Article ID: JHEP02(2024)129
arXiv:
hep-ph
2301.03816
Copyrights:
The Author(s)
Licence:
CC-BY-4.0
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