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Search for primary photons at tens of PeV with the Pierre Auger Observatory

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F24%3A00635934" target="_blank" >RIV/68378271:_____/24:00635934 - isvavai.cz</a>

  • Result on the web

    <a href="https://pos.sissa.it/444/238/pdf" target="_blank" >https://pos.sissa.it/444/238/pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.444.0238" target="_blank" >10.22323/1.444.0238</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Search for primary photons at tens of PeV with the Pierre Auger Observatory

  • Original language description

    The observation of primary photons with energies around 1016 eV would be particularly interesting after the discovery of Galactic gamma-ray sources with spectra extending into the PeV range. Since photons are connected to the acceleration of charged particles, searches for photons enhance the multi-messenger understanding of cosmic-ray sources as well as of transient astrophysical phenomena, while offering wealthy connections to neutrino astronomy and dark matter. Additionally, diffuse photon fluxes are expected from cosmic-ray interactions with Galactic matter and background radiation fields. Previously, the energy domain between 1 and 200 PeV was only explored from the Northern Hemisphere. The Pierre Auger Observatory is the largest astroparticle experiment in operation and, thanks to its location, has a sizable exposure to the Southern sky, including the Galactic center region. In this contribution, we present the first search for photons from the Southern hemisphere between 50 and 200 PeV exploiting the Auger data acquired during ∼4 yr of operation. We describe the method to discriminate photons against the dominating hadronic background, it is based on the measurements of air showers taken with the low-energy extension of the Pierre Auger Observatory composed by 19 water-Cherenkov detectors spanning ∼2 km2 and an Underground Muon Detector. The search for a diffuse flux of photons is presented and its results are interpreted according to theoretical model predictions. This study extends the range of Auger photon searches to almost four decades in energy.

  • 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

    238

  • 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