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Probing the sources of ultra-high-energy cosmic rays-constraints from cosmic-ray measurements

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F25%3A00641932" target="_blank" >RIV/68378271:90232/25:00641932 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.3390/universe11100331" target="_blank" >https://doi.org/10.3390/universe11100331</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3390/universe11100331" target="_blank" >10.3390/universe11100331</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Probing the sources of ultra-high-energy cosmic rays-constraints from cosmic-ray measurements

  • Original language description

    Ultra-high-energy cosmic rays (UHECRs) are the most energetic particles known-and yet their origin is still an open question. However, with the precision and accumulated statistics of the Pierre Auger Observatory and the Telescope Array, in combination with advancements in theory and modeling-e.g., of the Galactic magnetic field-it is now possible to set solid constraints on the sources of UHECRs. The spectrum and composition measurements above the ankle can be well described by a population of extragalactic, homogeneously distributed sources emitting mostly intermediate-mass nuclei. Additionally, using the observed anisotropy in the arrival directions, namely the large-scale dipole > 8 EeV, as well as smaller-scale warm spots at higher energies, even more powerful constraints on the density and distribution of sources can be placed. Yet, open questions remain-like the striking similarity of the sources that is necessary to describe the rather pure mass composition above the ankle, or the origin of the highest energy events whose tracked back directions point toward voids. The current findings and possible interpretation of UHECR data will be presented in this review.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

  • Continuities

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Universe

  • ISSN

    2218-1997

  • e-ISSN

    2218-1997

  • Volume of the periodical

    11

  • Issue of the periodical within the volume

    10

  • Country of publishing house

    CH - SWITZERLAND

  • Number of pages

    30

  • Pages from-to

    331

  • UT code for WoS article

    001604537800001

  • EID of the result in the Scopus database

    2-s2.0-105020035615