UHECR results of combined analyses of TA and Auger experiments

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F23%3A00578889" target="_blank" >RIV/68378271:_____/23:00578889 - isvavai.cz</a>
Alternative codes found
RIV/61989592:15310/23:73622717
Result on the web
<a href="https://www.epj-conferences.org/articles/epjconf/pdf/2023/06/epjconf_ricap2022_04001.pdf" target="_blank" >https://www.epj-conferences.org/articles/epjconf/pdf/2023/06/epjconf_ricap2022_04001.pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/epjconf/202328004001" target="_blank" >10.1051/epjconf/202328004001</a>

Result language
angličtina
Original language name
UHECR results of combined analyses of TA and Auger experiments
Original language description
The origin of ultra-high-energy cosmic rays (UHECRs) is still unknown. Their sources are believed to be within the local universe (a few hundred megaparsecs), but deflections by intergalactic and Galactic magnetic fields prevent us from straightforwardly associating UHECRs to their sources based on their arrival directions, making their angular distribution mostly isotropic. At higher energies, the number of potential source candidates and the magnetic deflections are both expected to be smaller, but so is the available amount of statistics. Hence, it is interesting to perform searches for anisotropies using several different energy thresholds.
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
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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