Gamma-ray bursts as sources of ultra-high energy cosmic rays across the ankle
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00548562" target="_blank" >RIV/68378271:_____/19:00548562 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/358/196/pdf" target="_blank" >https://pos.sissa.it/358/196/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.358.0196" target="_blank" >10.22323/1.358.0196</a>
Alternative languages
Result language
angličtina
Original language name
Gamma-ray bursts as sources of ultra-high energy cosmic rays across the ankle
Original language description
The origin of Ultra-High Energy Cosmic Rays (UHECRs) is still unknown. Gamma-Ray Bursts (GRBs) are considered as potential sources as they belong to the most energetic events observed to date. However, conventional GRB scenarios are strongly constrained by the non-observation of associated astrophysical neutrinos. On the other hand, hidden accelerators such as low-luminosity GRBs (LLGRBs) can ameliorate the constraints. We show that the population of LLGRBs is not only consistent with current constraints, but can even describe the UHECR spectrum and composition across the ankle as well as neutrino data simultaneously.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
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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