Upper limits on the cosmic-ray luminosity of supernovae in nearby galaxies
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00566030" target="_blank" >RIV/68378271:_____/22:00566030 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.22323/1.395.0461" target="_blank" >http://dx.doi.org/10.22323/1.395.0461</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0461" target="_blank" >10.22323/1.395.0461</a>
Alternative languages
Result language
angličtina
Original language name
Upper limits on the cosmic-ray luminosity of supernovae in nearby galaxies
Original language description
Interactions between cosmic rays and also between cosmic rays and particles of the Cosmic Microwave Background and the Extragalactic Background Light produce charged and neutral pions. The mechanisms that can produce gamma-ray fluxes associated with cosmic rays are the decay of neutral pions, bremsstrahlung, and inverse Compton scattering from pions. These cascading processes show a correlation between the upper limit on the integral GeV-TeV gamma-ray flux and the upper limit on the UHECR luminosity, motivating the study of the multi-messengers to calculate luminosities of UHECRs for specific point sources.n
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
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of Science
ISBN
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ISSN
1824-8039
e-ISSN
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Number of pages
6
Pages from-to
461
Publisher name
Sissa Medilab srl
Place of publication
Trieste
Event location
Berlin
Event date
Jul 12, 2021
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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