Arrival directions of ultra-high-energy cosmic rays assuming heavy mass-composition

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F25%3A00644563" target="_blank" >RIV/68378271:_____/25:00644563 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/484/069/pdf" target="_blank" >https://pos.sissa.it/484/069/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.484.0069" target="_blank" >10.22323/1.484.0069</a>

Result language
angličtina
Original language name
Arrival directions of ultra-high-energy cosmic rays assuming heavy mass-composition
Original language description
The arrival directions of cosmic rays are influenced by the Galactic and extragalactic magnetic fields, particularly in scenarios involving a heavy mass composition of primary particles. Following recent studies, we assume a pure iron composition of cosmic rays above 40 EeV and simulate their propagation in the Galactic magnetic field using the new UF23 base model. We analyze the expected arrival direction patterns on Earth assuming multiple source catalogues, including nearby active galactic nuclei or starburst galaxies. We compare the resulting patterns from the simulations with the published arrival directions of cosmic rays with energies above 40 EeV.
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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