The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays
The result's identifiers
Result code in 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>
Result on the web
<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>
Alternative languages
Result language
angličtina
Original language name
The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays
Original language description
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.
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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