Ultra-high energy neutrinos: status and prospects
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00549403" target="_blank" >RIV/68378271:_____/18:00549403 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/301/1111/pdf" target="_blank" >https://pos.sissa.it/301/1111/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.301.1111" target="_blank" >10.22323/1.301.1111</a>
Alternative languages
Result language
angličtina
Original language name
Ultra-high energy neutrinos: status and prospects
Original language description
Despite decades of observation, the nature and origin of ultra-high energy cosmic rays (UHECR), with energies in the EeV range and above, remains unknown. The mere existence of UHECR implies that UHE neutrinos should also be produced, but at a level that remains uncertain due to the relatively poor knowledge of some key properties of the sources of UHECR. In the last few years, the IceCube and Pierre Auger observatories have started to constrain potential sources of UHECR through the non-observation of the so-called cosmogenic neutrinos expected to be produced in interactions of UHECR with the Cosmic Microwave Background.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10303 - Particles and field physics
Result continuities
Project
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Continuities
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Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of Science
ISBN
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ISSN
1824-8039
e-ISSN
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Number of pages
16
Pages from-to
1-16
Publisher name
Sissa Medilab srl
Place of publication
Trieste
Event location
Busan
Event date
Jul 10, 2017
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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