χaroν: a tool for neutrino flux generation from WIMPs

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    • uploaded July 7, 2021

    Discussion timeslot (ZOOM-Meeting): 16. July 2021 - 18:00
    ZOOM-Meeting URL: https://icrc2021.desy.de/pf_access_abstracts
    Corresponding Session: https://icrc2021-venue.desy.de/channel/Presenter-Forum-1-Evening-All-Categories/48
    Abstract:
    'Indirect searches for signatures of corpuscular dark matter have been performed using all cosmic messengers: gamma rays, cosmic rays, and neutrinos. The search for dark matter with neutrinos is important since they are the only courier that can reach detectors from dark matter processes in dense environments, such as the core of the Sun or Earth, or the edge of the observable Universe. One thing essential to experiments is the prediction of the neutrino signature in the detector. I will introduce χaroν, a software that bridges the dark sector and Standard Model by predicting neutrino fluxes from different celestial dark matter agglomerations in diverse scenarios. This package includes updated computation of neutrino production and propagation to the detector.'

    Authors: Qinrui Liu
    Co-Authors: Jeffrey Lazar | Carlos Arguelles | Ali Kheirandish
    Indico-ID: 1411
    Proceeding URL: https://pos.sissa.it/395/559

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    Presenter:

    Qinrui Liu


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