Cosmogenic gamma-rays and neutrinos constrain UHECR source models
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00549827" target="_blank" >RIV/68378271:_____/18:00549827 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/301/562/pdf" target="_blank" >https://pos.sissa.it/301/562/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.301.0562" target="_blank" >10.22323/1.301.0562</a>
Alternative languages
Result language
angličtina
Original language name
Cosmogenic gamma-rays and neutrinos constrain UHECR source models
Original language description
When ultra-high-energy cosmic rays (UHECRs) propagate through the universe they produce secondary neutrinos as well as photons, electrons and positrons (initiating electromagnetic cascades) in different kinds of interactions. These neutrinos and electromagnetic cascades are detected at Earth as isotropic extragalactic fluxes. The level of these fluxes can be predicted and used to constrain UHECR source models.
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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