Starburst Galaxies as possible sources of UHECRs and neutrinos

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00565591" target="_blank" >RIV/68378271:_____/22:00565591 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.22323/1.395.0959" target="_blank" >http://dx.doi.org/10.22323/1.395.0959</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0959" target="_blank" >10.22323/1.395.0959</a>

Result language
angličtina
Original language name
Starburst Galaxies as possible sources of UHECRs and neutrinos
Original language description
The coexistence of powerful accelerators of cosmic rays with intense background radiation fields creates unique conditions, where the Ultra-High-Energy Cosmic Rays (UHECRs) interactions could take place copiously and produce several secondary particles. In particular, such phenomena could explain the features observed in the UHECR spectrum measurements. This scenario is explored extending SimProp, a simulation code for UHECR extra-galactic propagation, allowing us to compute the interactions inside and outside the source. Inspired by recent results from the Pierre Auger Observatory on the anisotropy in the arrival directions of the highest energy cosmic-rays, the simulations are performed in the context of Starburst Galaxies, one of the most promising candidate sources.nn
Czech name
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Czech description
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Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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