Neural Networks aproach to event reconstruction for the GAPS experiment

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

    • 0 favorites

    • uploaded July 5, 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:
    'The General Antiparticle Spectrometer (GAPS) is a balloon-borne detector, whose first flight is scheduled in the austral summer 2022,and is designed to measure low energy ( smaller 0.25 GeV/n) cosmic antinuclei. A particular focus is on antideuterons, which are predicted to have an ultra-low astrophysical background as compared to signals from dark matter annihilation or decay in the Galactic halo. GAPS uses a novel technique for particle identification based on the formation and decay of exotic atoms. To achieve sufficient rejection power for particle identification, an accurate determination of several fundamental quantities is needed. The precise reconstruction of the energy deposition pattern on the primary track is a particularly intricate problem and we exhibit a strategy devised to solve this using modern machine learning techniques. In the future, this approach can be used for particle identification. Here, we present preliminary results of these efforts obtained from simulated data.'

    Authors: Nadir Marcelli
    Collaboration: GAPS

    Indico-ID: 428
    Proceeding URL: https://pos.sissa.it/395/099

    Tags:
    Presenter:

    Nadir Marcelli


    Additional files

    More Media in "Cosmic Ray Direct"