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Deflections of UHECRs in the Galactic magnetic field

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00539838" target="_blank" >RIV/68378271:_____/19:00539838 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1088/1475-7516/2019/05/004" target="_blank" >https://doi.org/10.1088/1475-7516/2019/05/004</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/1475-7516/2019/05/004" target="_blank" >10.1088/1475-7516/2019/05/004</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Deflections of UHECRs in the Galactic magnetic field

  • Original language description

    We report results of the first comprehensive, high resolution study of the deflections of UHECRs using a realistic model of the Galactic magnetic field and extending to sufficiently low rigidities, R (math)E/Z >= 10(18) V, to describe Fe in the UHE energy range above similar to 55 EeV, or the mixed composition reported by the Pierre Auger Collaboration at the energy of the observed dipole anisotropy. We use the Jansson-Farrar (JF12) model, which has both a large scale coherent and a structured random component, and determine deflections for fifteen rigidities from 10(18.0) to 10(20.0) V, for two different coherence length choices for the random component, L-coh = 30 pc and 100 pc. We also check the sensitivity of UHECR deflections to the particular realization of the random field, for 3 rigidity values. For each rigidity and field model studied, the UHECR arrival direction distribution is determined for an arbitrary source direction, by inverting the trajectories of > 5 x 10(7) isotropically-distributed anti-CRs of the given rigidity, which we backtrack using the code CRT. We present skyplots and tables characterizing the arrival directions, for representative 1 degrees sources.

  • 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

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Journal of Cosmology and Astroparticle Physics

  • ISSN

    1475-7516

  • e-ISSN

  • Volume of the periodical

    2019

  • Issue of the periodical within the volume

    5

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    55

  • Pages from-to

    1-55

  • UT code for WoS article

    000466899500002

  • EID of the result in the Scopus database

    2-s2.0-85069652721