Cosmic ray anisotropies from transient extragalactic sources
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F21%3A00546090" target="_blank" >RIV/68378271:_____/21:00546090 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1103/PhysRevD.103.023012" target="_blank" >https://doi.org/10.1103/PhysRevD.103.023012</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1103/PhysRevD.103.023012" target="_blank" >10.1103/PhysRevD.103.023012</a>
Alternative languages
Result language
angličtina
Original language name
Cosmic ray anisotropies from transient extragalactic sources
Original language description
We study the spectrum and anisotropies of ultrahigh energy cosmic ray transient sources, accounting for the effects of their propagation through the turbulent extragalactic magnetic fields. We consider either bursting sources or sources emitting since a given initial time. We analyze in detail the transition between the diffusive and the quasirectilinear regimes, describing some new features that could be present.
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
—
Continuities
—
Others
Publication year
2021
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
ISSN
2470-0010
e-ISSN
2470-0029
Volume of the periodical
103
Issue of the periodical within the volume
2
Country of publishing house
US - UNITED STATES
Number of pages
12
Pages from-to
023012
UT code for WoS article
000606970000003
EID of the result in the Scopus database
2-s2.0-85099314163