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UCLA Dark Matter 2025

24–27 Mar 2025
UCLA Physics and Astronomy Building 1-425
US/Pacific timezone

darkmatter@physics.ucla.edu

Session

SESSION 4: Direct Dark Matter Detection (CHAIR: Alvine Kamaha -UCLA)

24 Mar 2025, 15:50
UCLA Physics and Astronomy Building 1-425

UCLA Physics and Astronomy Building 1-425

475 Portola Plaza, Los Angeles, CA 90095 darkmatter@physics.ucla.edu

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  1. 193. Direct Detection with Xenon
    Elena Aprile
    24/03/2025, 15:50
    Talk

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  2. 194. Direct Detection with Argon
    Cristiano Galbiati
    24/03/2025, 16:15
    Talk

    NA

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  3. 195. Direct Detection with Cryogenic Solid State Detectors
    Sunil Golwala
    24/03/2025, 16:40
    Talk

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  4. 196. The Status of Sub-GeV Direct Detection
    Rouven Essig
    24/03/2025, 17:05
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  5. 6. PaleoDetectors (Ancient Minerals from Deep Underground)
    Prof. Katherine Freese (University of Texas)
    24/03/2025, 17:30
    Talk

    Paleo-detectors are a proposed experimental technique to search for dark matter (DM). In lieu of the conventional approach of operating a tonne-scale real-time detector to search for DM-induced nuclear recoils, paleo-detectors take advantage of small samples of naturally occurring rocks on Earth that have been deep underground (≳5 km), accumulating nuclear damage tracks from recoiling nuclei...

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