The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays

Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00548652" target="_blank" >RIV/68378271:_____/19:00548652 - isvavai.cz</a>
Výsledek na webu
<a href="https://pos.sissa.it/358/254/pdf" target="_blank" >https://pos.sissa.it/358/254/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.358.0254" target="_blank" >10.22323/1.358.0254</a>

Jazyk výsledku
angličtina
Název v původním jazyce
The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays
Popis výsledku v původním jazyce
Auger data show evidence for a correlation between ultrahigh-energy cosmic rays (UHECRs) and nearby starburst galaxies. This intriguing correlation is consistent with data collected by the Telescope Array, which have revealed a much more pronounced directional “hot spot” in arrival directions not far from the starburst galaxy M82. In this work, we assume starbursts are sources of UHECRs and investigate the prospects to use the observed distribution of UHECR arrivalndirections to constrain Galactic magnetic field models.
Název v anglickém jazyce
The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays
Popis výsledku anglicky
Auger data show evidence for a correlation between ultrahigh-energy cosmic rays (UHECRs) and nearby starburst galaxies. This intriguing correlation is consistent with data collected by the Telescope Array, which have revealed a much more pronounced directional “hot spot” in arrival directions not far from the starburst galaxy M82. In this work, we assume starbursts are sources of UHECRs and investigate the prospects to use the observed distribution of UHECR arrivalndirections to constrain Galactic magnetic field models.

Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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