The all-particle cosmic ray energy spectrum measured with HAWC

Video Player is loading.
Loaded: 0%
Remaining Time 0:00
1x
  • Quality
    • 144 views

    • 0 favorites

    • uploaded July 7, 2021

    Discussion timeslot (ZOOM-Meeting): 14. July 2021 - 12:00
    ZOOM-Meeting URL: https://desy.zoom.us/j/92210078166
    ZOOM-Meeting ID: 92210078166
    ZOOM-Meeting Passcode: ICRC2021
    Corresponding Session: https://icrc2021-venue.desy.de/channel/04-CR-Energy-Spectrum-CRI/91
    Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-03/4

    Abstract:
    "Thanks to recent technological development, a new generation of experiments have been developed with more sensitivity in the energy interval from 10 TeV to 1 PeV, such as HAWC. Due to its designs and high altitude, the HAWC air shower observatory can provide a bridge between the data from direct and indirect cosmic ray detectors. In 2017 the HAWC collaboration published their first results on the energy spectrum of cosmic rays, in the range from 10 to 500 TeV. This work updates these results by extending the energy interval of the measured all-particle cosmic-ray energy spectrum up to 1 PeV. The energy spectrum was obtained from the analysis of two years of HAWC's data using an unfolding method. We employed the QGSJET-II-04 model for the energy calibration and the spectrum reconstruction. The results confirm the presence of a knee like feature around 45 TeV, which was reported by the HAWC collaboration in 2017."

    Authors: Jorge Antonio Morales-Soto | Juan Carlos Arteaga-Velázquez | for the HAWC Collaboration
    Collaboration: HAWC

    Indico-ID: 731
    Proceeding URL: https://pos.sissa.it/395/330

    Tags:
    Presenter:

    Jorge Antonio Morales-Soto


    Additional files

    More Media in "Cosmic Ray Indirect"