高能与超高能中微子
高能物理 - 唯象学
2022-07-14 v2 高能天体物理现象
高能物理 - 实验
摘要
天体物理中微子是探测天体粒子物理与高能物理的极佳探针。其能量远超太阳、超新星、大气与加速器产生的中微子，高能与超高能中微子可探测从 TeV 能标到 EeV 能标及更高尺度下的基础物理。通过其产生机制及在宇宙学距离上的传播，它们对标准模型之内与之外的物理均敏感。由于能洞察对电磁辐射不透明的区域，它们携带着关于极端非热源的独特信息。本白皮书描述了天体物理中微子观测在当今及未来数年中为天体物理与高能物理带来的机遇。
引用
@article{arxiv.2203.08096,
title = {High-Energy and Ultra-High-Energy Neutrinos},
author = {Markus Ackermann and Sanjib K. Agarwalla and Jaime Alvarez-Muñiz and Rafael Alves Batista and Carlos A. Argüelles and Mauricio Bustamante and Brian A. Clark and Austin Cummings and Sudipta Das and Valentin Decoene and Peter B. Denton and Damien Dornic and Zhan-Arys Dzhilkibaev and Yasaman Farzan and Alfonso Garcia and Maria Vittoria Garzelli and Christian Glaser and Aart Heijboer and Jörg R. Hörandel and Giulia Illuminati and Yu Seon Jeong and John L. Kelley and Kevin J. Kelly and Ali Kheirandish and Spencer R. Klein and John F. Krizmanic and Michael J. Larson and Lu Lu and Kohta Murase and Ashish Narang and Nepomuk Otte and Remy L. Prechelt and Steven Prohira and Mary Hall Reno and Elisa Resconi and Marcos Santander and Olga Vasil'evna Suvorova and Victor B. Valera and Justin Vandenbroucke and Lawrence Wiencke and Stephanie Wissel and Shigeru Yoshida and Tianlu Yuan and Enrique Zas and Pavel Zhelnin and Bei Zhou},
journal= {arXiv preprint arXiv:2203.08096},
year = {2022}
}
备注
Contribution to Snowmass 2021, updated to include community feedback