Cosmogenic neutrinos challenge the cosmic ray proton dip model
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00549480" target="_blank" >RIV/68378271:_____/18:00549480 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/301/589/pdf" target="_blank" >https://pos.sissa.it/301/589/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.301.0589" target="_blank" >10.22323/1.301.0589</a>
Alternative languages
Result language
angličtina
Original language name
Cosmogenic neutrinos challenge the cosmic ray proton dip model
Original language description
The origin and composition of ultra-high-energy cosmic rays (UHECRs) remain a mystery. The proton dip model describes the shape of the cosmic ray spectrum above 109 GeV by the effect of a pure proton spectrum propagating through the cosmic microwave background. In these interactions secondary neutrinos are produced.n
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
8
Pages from-to
1-8
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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