Jun 2 – 6, 2025
Santander, Spain
Europe/Madrid timezone

Session

Tuesday Morning I

Jun 3, 2025, 10:00 AM
Santander, Spain

Santander, Spain

Gran Hotel Victoria C. María Luisa Pelayo, 38 39005 Santander Cantabria, Spain

Presentation materials

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  1. Dr Amy Cottle (University College London)
    6/3/25, 10:00 AM
    DM Direct Detection
    Invited Talk

    Direct detection experiments aim to shed light on the thus far elusive nature of dark matter through measuring its potential interactions with ordinary matter. This talk will provide an overview of these experiments and the status of the field. After briefly summarising the possible dark matter candidates, I will cover some of the detection strategies and recent results, before discussing the...

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  2. Paulo Brás (LIP)
    6/3/25, 10:35 AM
    DM Direct Detection
    Contributed Talk

    The LUX-ZEPLIN (LZ) experiment is located at the Sanford Underground Research Facility in Lead, South Dakota. LZ is primarily designed to detect interactions of dark matter in the form of weakly-interacting massive particles (WIMPs) using a 7 tonne dual-phase xenon time projection chamber (TPC). LZ has been acquiring science data since 2021 under stable operating conditions. Now, with a...

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  3. Kai Böse (Max-Planck-Institut für Kernphysik)
    6/3/25, 10:55 AM
    DM Direct Detection
    Contributed Talk

    Direct detection experiments look for scattering events of dark matter with known Standard Model particles. Scattering on heavy nuclei is a promising approach to searching for heavy (above a few GeV) dark matter candidates. Liquid noble elements, like xenon, are especially suited because of their inert behavior, ability to be purified and be low in radioactivity.
    XENONnT is the result of two...

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  4. Samir Banik
    6/3/25, 11:15 AM
    DM Direct Detection
    Contributed Talk

    Cryogenic Rare Event Search with Superconducting Thermometers (CRESST) is a direct dark matter (DM) detection experiment located in the Laboratori Nazionali del Gran Sasso (LNGS) in Italy. The experiment operates scintillating crystals at cryogenic temperatures to search for nuclear recoils from DM particles and has achieved a threshold of $\sim$10 eV in its third phase (CRESST III). The...

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