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Simulations and background estimate for the DAMIC-M experiment

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  • Additional Information
    • Contributors:
      Laboratoire de physique subatomique et des technologies associées (SUBATECH); Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST); Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique); Institut Mines-Télécom Paris (IMT)-Institut Mines-Télécom Paris (IMT); Université de Nantes (UN); CNRS-University Chicago cooperation
    • Publication Information:
      HAL CCSD
      Società Italiana di Fisica (Bologna)
    • Publication Date:
      2021
    • Collection:
      Ecole des Mines de Nantes: HAL
    • Abstract:
      International audience ; DAMIC-M (Dark Matter in CCDs at Modane) is a near-future experiment aiming to search for low-mass dark matter particles through their interactions with the silicon nucleus or electrons in the bulk of charge-coupled devices (CCDs). With respect to its predecessor DAMIC at SNOLAB, DAMIC-M will have a 25 times larger detector mass and will achieve sub-electron readout noise thanks to the use of the so-called skipper CCDs. With these novelties, DAMIC-M will be sensitive to WIMPS with masses below 10 GeV and it will be leading the search of MeV-scale hidden sector candidates and eV-scale hidden photons. To achieve these results, DAMIC-M requires a radiogenic background rate of a fraction of decays/keV/kg/day. Thus, an extensive campaign of innovation of the detector technology and design is ongoing. Simulations are being exploited to optimize the detector design and drive the material selection and handling. This proceedings provides a comprehensive overview of the explored detector designs, the corresponding estimated backgrounds, and the strategies for its mitigation.
    • Relation:
      hal-03512701; https://hal.science/hal-03512701; https://hal.science/hal-03512701/document; https://hal.science/hal-03512701/file/ncc12343.pdf; INSPIRE: 2009915
    • Accession Number:
      10.1393/ncc/i2022-22006-y
    • Online Access:
      https://hal.science/hal-03512701
      https://hal.science/hal-03512701/document
      https://hal.science/hal-03512701/file/ncc12343.pdf
      https://doi.org/10.1393/ncc/i2022-22006-y
    • Rights:
      info:eu-repo/semantics/OpenAccess
    • Accession Number:
      edsbas.D1EDE05