Constraining the origin of UHECRs and astrophysical neutrinos

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    • uploaded July 7, 2021

    Discussion timeslot (ZOOM-Meeting): 13. 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/02-Constraining-UHECR-sources-CRI/63
    Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-03/4

    Abstract:
    'We constrain properties of ultrahigh energy cosmic ray source environments (and potentially astrophysical neutrino sources), including their photon temperature, gas density, size, magnetic field strength and coherence length, using UHECR and neutrino spectra and composition. Our analysis represents a new type of information on UHECR sources, independent of the mechanism responsible for the UHECR acceleration. We also explore the possibility of a common origin of UHECRs and astrophysical neutrinos and further constrain sources which are consistent with this possibility. We show that the common origin hypothesis can only be satisfied for certain hadronic interaction models, showing that multimessenger analyses have the power to also constrain hadronic physics beyond LHC energies.'

    Authors: Marco Muzio
    Co-Authors: Glennys Farrar | Michael Unger
    Indico-ID: 1410
    Proceeding URL: https://pos.sissa.it/395/1021

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    Presenter:

    Marco Muzio


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