Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F20%3A00536210" target="_blank" >RIV/68378271:_____/20:00536210 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1103/PhysRevD.102.023034" target="_blank" >https://doi.org/10.1103/PhysRevD.102.023034</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1103/PhysRevD.102.023034" target="_blank" >10.1103/PhysRevD.102.023034</a>
Alternative languages
Result language
angličtina
Original language name
Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts
Original language description
The Pierre Auger Collaboration has provided a compelling indication for a possible correlation between the arrival directions of ultrahigh-energy cosmic rays and nearby starburst galaxies. Herein we show how the latest large-scale modeling of starburst galaxies is compatible with the cosmic rays producing the anisotropy signal being accelerated at the terminal shock of superwinds.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
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
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Physical Review D: Particles, Fields, Gravitation and Cosmology
ISSN
1550-7998
e-ISSN
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Volume of the periodical
102
Issue of the periodical within the volume
2
Country of publishing house
US - UNITED STATES
Number of pages
9
Pages from-to
1-9
UT code for WoS article
000552579500004
EID of the result in the Scopus database
2-s2.0-85092936112