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Depth of maximum of air-shower profiles above 1017.8 eV measured with the fluorescence detector of the Pierre Auger Observatory and mass composition implications

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F24%3A00635907" target="_blank" >RIV/68378271:_____/24:00635907 - isvavai.cz</a>

  • Result on the web

    <a href="https://pos.sissa.it/444/319/pdf" target="_blank" >https://pos.sissa.it/444/319/pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.444.0319" target="_blank" >10.22323/1.444.0319</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Depth of maximum of air-shower profiles above 1017.8 eV measured with the fluorescence detector of the Pierre Auger Observatory and mass composition implications

  • Original language description

    After seventeen years of operation, the first phase of measurements at the Pierre Auger Observatory finished and the process of upgrading it began. In this work, we present distributions of the depth of air-shower maximum, Xmax , using profiles measured with the fluorescence detector of the Pierre Auger Observatory. The analysis is based on the Phase I data collected from 01 December 2004 to 31 December 2021. The Xmax measurements take advantage of an improved evaluation of the vertical aerosol optical depth and reconstruction of the shower profiles. We present the energy dependence of the mean and standard deviation of the Xmax distributions above 1017.8 eV. Both Xmax moments are corrected for detector effects and interpreted in terms of the mean logarithmic mass and variance of the masses by comparing them to the predictions of post-LHC hadronic interaction models. We corroborate our earlier findings regarding the change of the elongation rate of the mean Xmax at 1018.3 eV with higher significance. We also confirm, with four more years of data compared to the last results presented in 2019, that around the ankle in the cosmic rays spectrum, the proton component gradually disappears and that intermediate mass nuclei dominate the composition at ultra-high energies.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of Science

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

  • Number of pages

    13

  • Pages from-to

    319

  • Publisher name

    Sissa Medilab srl

  • Place of publication

    Trieste

  • Event location

    Nagoya

  • Event date

    Jul 26, 2023

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article