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Magnificent CEvNS 2019

9–11 Nov 2019
The PIT
America/New_York timezone

Session

Noble-element detectors and dark matter

10 Nov 2019, 11:00
The PIT

The PIT

462 W Franklin St Chapel Hill, NC 27516 USA

Conveners

Noble-element detectors and dark matter

  • Matthew Green (NC State University)

Noble-element detectors and dark matter

  • Louis Strigari (Texas A&M)

Presentation materials

There are no materials yet.

  1. 13. Prospects of CEvNS Detection with the XENON100 Detector
    Kaixuan Ni (University of California San Diego)
    10/11/2019, 11:00
    Invited

    Two-phase xenon detectors are being actively developed over the last decade and made substantial improvement of search sensitivity for WIMP dark matter. These detectors, operated in time projection chamber (TPC) mode, strongly suppress the electronic recoil background, making it possible to detect CEvNS of neutrinos at the Spallation Neutron Source (SNS). In addition, two-phase xenon detectors...

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  2. 44. Progress and plans for DARKSIDE and QF measurements in LAr
    Claudio Savarese
    10/11/2019, 11:20
    Invited

    Progress and plans for DARKSIDE and QF measurements in LAr.

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  3. 57. Searching for Sterile Neutrinos with Coherent Captain Mills
    Mr Edward Dunton (LANL)
    10/11/2019, 11:40
    Invited

    Despite evidence from LSND and MiniBooNE for sterile neutrinos at $Δm^2$ = 1 $eV^2$ in electron neutrino appearance experiments, corresponding muon-neutrino disappearance experiments have shown no anomalies. However, these experiments have been performed at a different energy scale compared to LSND and MiniBooNE. Coherent CAPTAIN Mills (CCM) is an experiment at the Lujan Center at LANSCE that...

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  4. 32. Future LAr program in COHERENT
    Rex Tayloe (Indiana U.)
    10/11/2019, 12:00
    Invited

    Future LAr program in COHERENT.

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  5. 36. COHERENT sensitivity to DM
    Daniel Pershey (Duke University)
    10/11/2019, 12:20
    Invited

    We will discuss the sensitivity of the COHERENT experiment to test sub-GeV dark matter candidates that may be produced by the SNS and highlight the advantages of using CEvNS detectors for these searches. We also will show strategies within reach of the next generation of detectors that maximize discovery potential for such detectors.

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  6. 40. Status and future plans of SuperCDMS
    Rupak Mahapatra (Texas A&M University)
    10/11/2019, 14:30

    Status and future plans of SuperCDMS.

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  7. 63. Dark matter and neutrino search with the LZ experiment
    Dr Jingke Xu (Lawrence Livermore National Laboratory)
    10/11/2019, 14:50
    Invited

    The LZ dark matter detector is currently under construction at the 4850 level of the Sanford Underground Research Facility (SURF) in Lead, SD. The experiment will contain 7 tonnes of pure xenon in a dual-phase Time Project Chamber (TPC) – a technology that has demonstrated very high sensitivities to hypothetical dark matter interactions. LZ is projected to reach unprecedented sensitivities for...

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  8. 7. The CYGNUS Directional Dark Matter Experiment and Neutrino-Nucleus Scattering
    Prof. Neil Spooner (University of Sheffield)
    10/11/2019, 15:10
    Invited

    CYGNUS is a coordinated effort by dark matter direct search groups interested in directional signals, working towards design and build of a global network of directional WIMP experiments able to probe below the neutrino floor. As such, sensitivity is required to detection and measurement of Solar neutrino-nucleus scattering with directional information. The proposed technology is that of low...

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