High-Energy and Ultra-High-Energy Neutrinos: A Snowmass White Paper
High-Energy and Ultra-High-Energy Neutrinos: A Snowmass White Paper
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DOI：
10.1016/j.jheap.2022.08.001
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发表时间：
2022-08
影响因子：
3.8
通讯作者：
M. Ackermann;M. Bustamante;Lu Lu-Lu;N. Otte;M. Reno;S. Wissel;S. Agarwalla;J. Alvarez-Muñiz;R. A. Batista;C. Argüelles;B. Clark;A. Cummings;Sudipta Das;V. Decoene;P. Denton;D. Dornic;Z. Dzhilkibaev;Y. Farzan;Alfonso Garcia;M. Garzelli;C. Glaser;A. Heijboer;J. Hörandel;G. Illuminati;Yu Seon Jeong;J. Kelley;K. Kelly;A. Kheirandish;S. Klein;J. Krizmanic;M. Larson;K. Murase;Ashish Narang;R. Prechelt;S. Prohira;E. Resconi;M. Santander;Víctor B. Valera;J. Vandenbroucke;Olga Vasil'evna Suvorova;L. Wiencke;S. Yoshida;T. Yuan;E. Zas;P. Zhelnin;Bei Zhou;L. Anchordoqui;Y. Ashida;M. Bagheri;A. Balagopal;V. Basu;James Beatty;K. Bechtol;N. Bell;Abigail C. Bishop;J. Book;Anthony Brown;A. Burgman;M. Campana;N. Chau;Thomas Y. Chen;Alan Coleman;A. Connolly;J. Conrad;P. Correa;Cyril Creque-Sarbinowski;Z. Curtis-Ginsberg;P. Dasgupta;S. de Kockere;K. de Vries;C. Deaconu;A. Desai;T. DeYoung;A. di Matteo;D. Elsaesser;P. Fürst;Lung Fan Kwok;A. Fedynitch;Derek Fox;E. Ganster;M. H. Minh;C. Haack;Steffen Hallman;F. Halzen;A. Haungs;A. Ishihara;E. Judd;T. Karg;A. Karle;T. Katori;A. Kochocki;C. Kopper;M. Kowalski;I. Kravchenko;N. Kurahashi;M. Lamoureux;H. L. Vargas;M. Lincetto;Qinrui Liu;J. Madsen;Y. Makino;J. Mammo;Z. Márka;E. Mayotte;K. Meagher;M. Meier;L. Miramonti;M. Moulai;K. Mulrey;M. Muzio;R. Naab;A. Nelles;W. Nichols;A. Nozdrina;E. O’Sullivan;Vivian OD́ell;Jesse Osborne;V. Pandey;E. Paudel;A. Pizzuto;M. Plum;Carlos Pobes Aranda;L. Pyras;Christoph Raab;Z. Rechav;J. Rojo;O. R. Matamala;P. Savina;F. Schroeder;L. Schumacher;S. Sciutto;S. Sclafani;Mohammad Ful Hossain Seikh;Manuel Silva;Rajeev Singh;Daniel Smith;Samuel Timothy Spencer;R. Springer;J. Stachurska;O. Suvorova;I. Taboada;S. Toscano;M. Tueros;J. P. Twagirayezu;N. van Eijndhoven;P. Veres;A. Vieregg;Winnie Wang;N. Whitehorn;W. Winter;E. Yildizci;Shiqi Yu
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文献类型：
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作者：
M. Ackermann;M. Bustamante;Lu Lu-Lu;N. Otte;M. Reno;S. Wissel;S. Agarwalla;J. Alvarez-Muñiz;R. A. Batista;C. Argüelles;B. Clark;A. Cummings;Sudipta Das;V. Decoene;P. Denton;D. Dornic;Z. Dzhilkibaev;Y. Farzan;Alfonso Garcia;M. Garzelli;C. Glaser;A. Heijboer;J. Hörandel;G. Illuminati;Yu Seon Jeong;J. Kelley;K. Kelly;A. Kheirandish;S. Klein;J. Krizmanic;M. Larson;K. Murase;Ashish Narang;R. Prechelt;S. Prohira;E. Resconi;M. Santander;Víctor B. Valera;J. Vandenbroucke;Olga Vasil'evna Suvorova;L. Wiencke;S. Yoshida;T. Yuan;E. Zas;P. Zhelnin;Bei Zhou;L. Anchordoqui;Y. Ashida;M. Bagheri;A. Balagopal;V. Basu;James Beatty;K. Bechtol;N. Bell;Abigail C. Bishop;J. Book;Anthony Brown;A. Burgman;M. Campana;N. Chau;Thomas Y. Chen;Alan Coleman;A. Connolly;J. Conrad;P. Correa;Cyril Creque-Sarbinowski;Z. Curtis-Ginsberg;P. Dasgupta;S. de Kockere;K. de Vries;C. Deaconu;A. Desai;T. DeYoung;A. di Matteo;D. Elsaesser;P. Fürst;Lung Fan Kwok;A. Fedynitch;Derek Fox;E. Ganster;M. H. Minh;C. Haack;Steffen Hallman;F. Halzen;A. Haungs;A. Ishihara;E. Judd;T. Karg;A. Karle;T. Katori;A. Kochocki;C. Kopper;M. Kowalski;I. Kravchenko;N. Kurahashi;M. Lamoureux;H. L. Vargas;M. Lincetto;Qinrui Liu;J. Madsen;Y. Makino;J. Mammo;Z. Márka;E. Mayotte;K. Meagher;M. Meier;L. Miramonti;M. Moulai;K. Mulrey;M. Muzio;R. Naab;A. Nelles;W. Nichols;A. Nozdrina;E. O’Sullivan;Vivian OD́ell;Jesse Osborne;V. Pandey;E. Paudel;A. Pizzuto;M. Plum;Carlos Pobes Aranda;L. Pyras;Christoph Raab;Z. Rechav;J. Rojo;O. R. Matamala;P. Savina;F. Schroeder;L. Schumacher;S. Sciutto;S. Sclafani;Mohammad Ful Hossain Seikh;Manuel Silva;Rajeev Singh;Daniel Smith;Samuel Timothy Spencer;R. Springer;J. Stachurska;O. Suvorova;I. Taboada;S. Toscano;M. Tueros;J. P. Twagirayezu;N. van Eijndhoven;P. Veres;A. Vieregg;Winnie Wang;N. Whitehorn;W. Winter;E. Yildizci;Shiqi Yu
天体物理中微子是天体粒子物理和高能物理的优秀探测器。高能和超高能中微子的能量远远超过太阳、超新星、大气和加速器中微子，它们探测从TeV尺度到EeV尺度甚至更高的基础物理。它们通过其产生机制和在宇宙学距离上的传播对标准模型内外的物理学都很敏感。它们通过洞察对电磁辐射不透明的区域来携带关于其极端非热源的独特信息。这篇白色论文描述了天体物理学中微子观测为今天和未来几年的天体物理学和高能物理学提供的机会。
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years.