Abstract
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.
Original language | English |
---|---|
Pages (from-to) | 55-110 |
Number of pages | 56 |
Journal | Journal of High Energy Astrophysics |
Volume | 36 |
Early online date | 5 Sept 2022 |
DOIs | |
Publication status | Published - Nov 2022 |
Fingerprint
Dive into the research topics of 'High-energy and ultra-high-energy neutrinos: A Snowmass white paper'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver
}
In: Journal of High Energy Astrophysics, Vol. 36, 11.2022, p. 55-110.
Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - High-energy and ultra-high-energy neutrinos
T2 - A Snowmass white paper
AU - Ackermann, Markus
AU - Bustamante, Mauricio
AU - Lu, Lu
AU - Otte, Nepomuk
AU - Reno, Mary Hall
AU - Wissel, Stephanie
AU - Agarwalla, Sanjib K.
AU - Alvarez-Muñiz, Jaime
AU - Alves Batista, Rafael
AU - Argüelles, Carlos A.
AU - Clark, Brian A.
AU - Cummings, Austin
AU - Das, Sudipta
AU - Decoene, Valentin
AU - Denton, Peter B.
AU - Dornic, Damien
AU - Dzhilkibaev, Zhan Arys
AU - Farzan, Yasaman
AU - Garcia, Alfonso
AU - Garzelli, Maria Vittoria
AU - Glaser, Christian
AU - Heijboer, Aart
AU - Hörandel, Jörg R.
AU - Illuminati, Giulia
AU - Seon Jeong, Yu
AU - Kelley, John L.
AU - Kelly, Kevin J.
AU - Kheirandish, Ali
AU - Klein, Spencer R.
AU - Krizmanic, John F.
AU - Larson, Michael J.
AU - Murase, Kohta
AU - Narang, Ashish
AU - Prechelt, Remy L.
AU - Prohira, Steven
AU - Resconi, Elisa
AU - Santander, Marcos
AU - Valera, Victor B.
AU - Vandenbroucke, Justin
AU - Vasil'evna Suvorova, Olga
AU - Wiencke, Lawrence
AU - Yoshida, Shigeru
AU - Yuan, Tianlu
AU - Zas, Enrique
AU - Zhelnin, Pavel
AU - Zhou, Bei
AU - Anchordoqui, Luis A.
AU - Ashida, Yosuke
AU - Bagheri, Mahdi
AU - Balagopal, Aswathi
AU - Basu, Vedant
AU - Beatty, James
AU - Bechtol, Keith
AU - Bell, Nicole
AU - Bishop, Abigail
AU - Book, Julia
AU - Brown, Anthony
AU - Burgman, Alexander
AU - Campana, Michael
AU - Chau, Nhan
AU - Chen, Thomas Y.
AU - Coleman, Alan
AU - Connolly, Amy
AU - Conrad, Janet M.
AU - Correa, Pablo
AU - Creque-Sarbinowski, Cyril
AU - Curtis-Ginsberg, Zachary
AU - Dasgupta, Paramita
AU - De Kockere, Simon
AU - de Vries, Krijn
AU - Deaconu, Cosmin
AU - Desai, Abhishek
AU - DeYoung, Tyce
AU - di Matteo, Armando
AU - Elsaesser, Dominik
AU - Fürst, Phillip
AU - Fan, Kwok Lung
AU - Fedynitch, Anatoli
AU - Fox, Derek
AU - Ganster, Erik
AU - Minh, Martin Ha
AU - Haack, Christian
AU - Hallman, Steffen
AU - Halzen, Francis
AU - Haungs, Andreas
AU - Ishihara, Aya
AU - Judd, Eleanor
AU - Karg, Timo
AU - Karle, Albrecht
AU - Katori, Teppei
AU - Kochocki, Alina
AU - Kopper, Claudio
AU - Kowalski, Marek
AU - Kravchenko, Ilya
AU - Kurahashi, Naoko
AU - Lamoureux, Mathieu
AU - León Vargas, Hermes
AU - Lincetto, Massimiliano
AU - Liu, Qinrui
AU - Madsen, Jim
AU - Makino, Yuya
AU - Mammo, Joseph
AU - Marka, Zsuzsa
AU - Mayotte, Eric
AU - Meagher, Kevin
AU - Meier, Maximilian
AU - Miramonti, Lino
AU - Moulai, Marjon
AU - Mulrey, Katharine
AU - Muzio, Marco
AU - Naab, Richard
AU - Nelles, Anna
AU - Nichols, William
AU - Nozdrina, Alisa
AU - O'Sullivan, Erin
AU - OD́ell, Vivian
AU - Osborne, Jesse
AU - Pandey, Vishvas
AU - Paudel, Ek Narayan
AU - Pizzuto, Alex
AU - Plum, Mattias
AU - Pobes Aranda, Carlos
AU - Pyras, Lilly
AU - Raab, Christoph
AU - Rechav, Zoe
AU - Rojo, Juan
AU - Romero Matamala, Oscar
AU - Savina, Pierpaolo
AU - Schroeder, Frank
AU - Schumacher, Lisa
AU - Sciutto, Sergio
AU - Sclafani, Stephen
AU - Ful Hossain Seikh, Mohammad
AU - Silva, Manuel
AU - Singh, Rajeev
AU - Smith, Daniel
AU - Spencer, Samuel Timothy
AU - Springer, Robert Wayne
AU - Stachurska, Juliana
AU - Suvorova, Olga
AU - Taboada, Ignacio
AU - Toscano, Simona
AU - Tueros, Matias
AU - Twagirayezu, Jean Pierre
AU - van Eijndhoven, Nick
AU - Veres, Péter
AU - Vieregg, Abigail
AU - Wang, Winnie
AU - Whitehorn, Nathan
AU - Winter, Walter
AU - Yildizci, Emre
AU - Yu, Shiqi
N1 - Funding Information: MA is supported by the Initiative and Networking Fund of the Helmholtz Association , the Deutsches Elektronen-Synchrotron (DESY). MB is supported by the Villum Fonden under project no. 29388 . LL is supported by the US National Science Foundation (US NSF)-Office of Polar Programs, the US NSF Physics Division through Awards PHY-1913607 and the Wisconsin Alumni Research Foundation . NO is supported by the US NSF through Award 2112769 . MHR is supported in part by the U.S. Department of Energy (US DOE) grant DE-SC-0010113 . SAW is supported by the US NSF through Awards 2111232 and CAREER 2033500 and NASA through Awards 80NSSC20K1288 , 80NSSC20K0925 , and 80NSSC20K0775 . SKA and AN acknowledge the financial support from the Swarnajayanti Fellowship Research Grant (File no. S̃B/SJF/2020-21/21 ) provided by the Science and Engineering Research Board (SERB) and Department of Science and Technology (DST), Govt. of India. SKA would like to thank the United States-India Educational Foundation for providing the financial support through the Fulbright-Nehru Academic and Professional Excellence Fellowship (Award No. 2710/F-N APE/2021 ). JAM and EZ have received financial support from Xunta de Galicia (Centro singular de investigación de Galicia accreditation 2019-2022), by European Union ERDF , and by the “María de Maeztu” Units of Excellence program MDM-2016-0692 and the Spanish Research State Agency , and from Ministerio de Ciencia e Innovación PID2019-105544GB-I00 and RED2018-102661-T (RENATA). RAB is funded by the “la Caixa” Foundation (ID 100010434 ) and the European Union's Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No 847648 , fellowship code LCF/BQ/PI21/11830030 . BAC thanks the National Science Foundation for support through the Astronomy and Astrophysics Postdoctoral Fellowship under Award AST-1903885 . PBD acknowledges support from the US DOE under Grant Contract DE-SC0012704 . YF would like to acknowledge support from the ICTP through the Associates Programme and from the Simons Foundation through grant number 284558FY19 . YSJ is supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government through Ministry of Science and ICT Grant 2021R1A2C1009296 . The work of SRK was supported in part by the US NSF under grant number PHY-1307472 and the US DOE under contract number DE-AC-76SF00098 . JFK acknowledges support by NASA grant 80NSSC19K0626 at the University of Maryland, Baltimore County and under proposal 17-APRA17-0066 at NASA/GSFC . ER is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) SFB 1258 , Cluster of Excellence 2094 ORIGINS , and the European Research Council (ERC) (Grant agreement No. 101053168 ). ZhD and OVS are supported by the Ministry of Education and Science of the Russian Federation within the financing program of large scientific projects of the “Science” National Project (grant no. 075-15-2020-778 ). The work of SY is supported by JSPS KAKENHI Grant No. 18H05206 . BZ is supported by the Simons Foundation . Publisher Copyright: © 2022 Elsevier B.V.
PY - 2022/11
Y1 - 2022/11
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=85137278323&partnerID=8YFLogxK
U2 - 10.1016/j.jheap.2022.08.001
DO - 10.1016/j.jheap.2022.08.001
M3 - Article
AN - SCOPUS:85137278323
SN - 2214-4048
VL - 36
SP - 55
EP - 110
JO - Journal of High Energy Astrophysics
JF - Journal of High Energy Astrophysics
ER -