DARWIN – a next-generation liquid xenon observatory for dark matter and neutrino physics

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    • uploaded July 1, 2021

    Discussion timeslot (ZOOM-Meeting): 13. July 2021 - 18:00
    ZOOM-Meeting URL: https://desy.zoom.us/j/96969970711
    ZOOM-Meeting ID: 96969970711
    ZOOM-Meeting Passcode: ICRC2021
    Corresponding Session: https://icrc2021-venue.desy.de/channel/42-Direct-Dark-Matter-Present-and-Future-DM/86
    Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-07/8

    Abstract:
    Benefiting from more than a decade of experience in WIMP searches with dual-phase xenon time projection chambers, the DARWIN (DARk matter WImp search with liquid xenoN) collaboration intends to build a next-generation detector involving 50 tonnes (40 tonnes active) of xenon. The primary goal of the observatory is to explore the entire experimentally accessible parameter space for WIMP masses above 5 GeV/c$^2$ down to the irreducible neutrino floor. With its low energy threshold and ultra-low background level, DARWIN will be an excellent platform to search for various other rare interactions. These include the neutrinoless double beta decay of $^{136}$Xe, a high-precision measurement of the low-energy solar neutrino flux, as well as searches for solar axions and axion-like-particles. In this talk, we will present the detector concept, the sensitivity to the various science channels, and ongoing RandD efforts.'

    Authors: Kevin Thieme
    Co-Authors: for the DARWIN Collaboration
    Collaboration: DARWIN

    Indico-ID: 589
    Proceeding URL: https://pos.sissa.it/395/548

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    Presenter:

    Kevin Thieme


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