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| 001 | 482712 | ||
| 005 | 20250724151846.0 | ||
| 024 | 7 | _ | |a 10.1016/j.jheap.2022.08.001 |2 doi |
| 024 | 7 | _ | |a Ackermann:2022rqc |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:2052677 |2 inspire |
| 024 | 7 | _ | |a 2214-4048 |2 ISSN |
| 024 | 7 | _ | |a 2214-4056 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2203.08096 |2 arXiv |
| 024 | 7 | _ | |a WOS:000890744900001 |2 WOS |
| 024 | 7 | _ | |a openalex:W4295354092 |2 openalex |
| 037 | _ | _ | |a PUBDB-2022-04914 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 088 | _ | _ | |a arXiv:2203.08096 |2 arXiv |
| 100 | 1 | _ | |a Ackermann, Markus |0 P:(DE-H253)PIP1014130 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 2022 Snowmass Summer Study |c Seattle |d 2022-07-17 - 2022-07-26 |w United States |
| 245 | _ | _ | |a High-energy and ultra-high-energy neutrinos: A Snowmass white paper |
| 260 | _ | _ | |a Amsterdam [u.a.] |c 2022 |b Elsevier |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Contribution to a conference proceedings |0 PUB:(DE-HGF)8 |2 PUB:(DE-HGF) |m contrib |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1664455416_15821 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a Contribution to Snowmass 2021, updated to include community feedback. Submitted to JHEApTanja, Volltext habe ich angefragt bei M. Ackermann. VG CarolaWaiting for fulltext |
| 520 | _ | _ | |a 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. |
| 536 | _ | _ | |a 613 - Matter and Radiation from the Universe (POF4-613) |0 G:(DE-HGF)POF4-613 |c POF4-613 |f POF IV |x 0 |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de |
| 650 | _ | 7 | |a neutrino: energy |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: energy: high |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: UHE |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: detector |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: propagation |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: decay |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: flux |2 INSPIRE |
| 650 | _ | 7 | |a WIMP: dark matter |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: supernova |2 INSPIRE |
| 650 | _ | 7 | |a ANITA |2 INSPIRE |
| 650 | _ | 7 | |a IceCube |2 INSPIRE |
| 650 | _ | 7 | |a KM3NeT |2 INSPIRE |
| 650 | _ | 7 | |a Baikal |2 INSPIRE |
| 650 | _ | 7 | |a numerical calculations |2 INSPIRE |
| 650 | _ | 7 | |a new physics |2 INSPIRE |
| 650 | _ | 7 | |a neutrino, UHE |2 INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-H253)IceCube-20150101 |5 EXP:(DE-H253)IceCube-20150101 |e IceCube South Pole Neutrino Observatory |x 0 |
| 700 | 1 | _ | |a Bustamante, Mauricio |0 M.Bustamante.1 |b 1 |
| 700 | 1 | _ | |a Lu, Lu |0 P:(DE-H253)PIP1033231 |b 2 |e Corresponding author |
| 700 | 1 | _ | |a Otte, Nepomuk |0 A.Nepomuk.Otte.1 |b 3 |e Corresponding author |
| 700 | 1 | _ | |a Reno, Mary Hall |0 M.H.Reno.1 |b 4 |e Corresponding author |
| 700 | 1 | _ | |a Wissel, Stephanie |0 S.A.Wissel.1 |b 5 |e Collaboration author |
| 700 | 1 | _ | |a Agarwalla, Sanjib K. |0 Sanjib.Kumar.Agarwalla.1 |b 6 |
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| 773 | _ | _ | |a 10.1016/j.jheap.2022.08.001 |g Vol. 36, p. 55 - 110 |0 PERI:(DE-600)2758722-8 |p 55 - 110 |t Journal of high energy astrophysics |v 36 |y 2022 |x 2214-4048 |
| 787 | 0 | _ | |a Ackermann, Markus et.al. |d 2022 |i IsParent |0 PUBDB-2022-04968 |r arXiv:2203.08096 |t High-energy and ultra-high-energy neutrinos: A Snowmass white paper |
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