Current constraints from cosmogenic neutrinos on the fraction of protons in UHECRs
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00548666" target="_blank" >RIV/68378271:_____/19:00548666 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/358/1025/pdf" target="_blank" >https://pos.sissa.it/358/1025/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.358.1025" target="_blank" >10.22323/1.358.1025</a>
Alternative languages
Result language
angličtina
Original language name
Current constraints from cosmogenic neutrinos on the fraction of protons in UHECRs
Original language description
Cosmogenic neutrinos are created when ultra-high-energy cosmic rays (UHECRs) interact with extragalactic photon backgrounds. In general, the expected flux of these cosmogenic neutrinos depends on multiple parameters, describing the sources and propagation of UHECRs. In our recent paper (van Vliet et al., 2019), we show that a `sweet spot` occurs at a neutrino energy of Eν∼1 EeV. At that energy the flux mainly depends on two parameters, the source evolution and the fraction of protons in UHECRs at Earth for Ep≳30 EeV.
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
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
PoS - 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
Madison, WI
Event date
Jul 24, 2021
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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