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Techniques for searching for anisotropy in the arrival directions of ultra-high energy cosmic rays

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F25%3A00641985" target="_blank" >RIV/68378271:90232/25:00641985 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1007/s13538-024-01640-6" target="_blank" >https://doi.org/10.1007/s13538-024-01640-6</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s13538-024-01640-6" target="_blank" >10.1007/s13538-024-01640-6</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Techniques for searching for anisotropy in the arrival directions of ultra-high energy cosmic rays

  • Original language description

    Understanding the origin and distribution of ultra-high-energy cosmic rays (UHECRs) remains a cornerstone challenge in astrophysics. These cosmic rays, with energies exceeding 8 EeV, provide insights into the most energetic phenomena in the universe. In this paper, we review and apply various statistical and analytical techniques to a simulated dataset to investigate the anisotropy in the arrival directions of UHECRs with energies exceeding 8 EeV. We simulate cosmic-ray events based on the distribution of local matter from the 2MASS Redshift Survey, supplemented with an isotropic background component, to create a robust dataset for analysis. Our methods include blind searches for excesses over the sky, Rayleigh analysis in right ascension, reconstruction of dipole and quadrupole moments using spherical harmonics, and the angular power spectrum technique — a method extensively utilized in cosmic microwave background studies — to assess anisotropies across multiple angular scales. The results underscore the potential of these methodologies to reveal significant anisotropies and contribute to our understanding of the possible extragalactic sources and propagation mechanisms of UHECRs.

  • 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

    Brazilian Journal of Physics

  • ISSN

    0103-9733

  • e-ISSN

    1678-4448

  • Volume of the periodical

    55

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    BR - BRAZIL

  • Number of pages

    8

  • Pages from-to

    9

  • UT code for WoS article

    001351523500001

  • EID of the result in the Scopus database

    2-s2.0-85209821969