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Dark Matter Interpretations for Direct Detection

9 August 2016
Lincoln College, Oxford
WET timezone

Session

Afternoon Session

9 Aug 2016, 13:30
Lincoln College, Oxford

Lincoln College, Oxford

Presentation materials

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  1. 9. Dark matter effective field theory scattering in the XE100 detector
    Ran Itay
    09/08/2016, 13:30
  2. 10. Prospects for dark matter detection with inelastic transitions of xenon
    Christopher McCabe
    09/08/2016, 14:00
    Dark matter can scatter and excite a nucleus to a low-lying excitation in a direct detection experiment. This signature is distinct from the canonical elastic scattering signal because the inelastic signal also contains the energy deposited from the subsequent prompt de-excitation of the nucleus. A measurement of the elastic and inelastic signal will allow a single experiment to distinguish...
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  3. 11. Leading corrections to spin-independent WIMP scattering off nuclei
    Javier Menéndez
    09/08/2016, 14:30
  4. 6. EFT/simplified models
    Mr Uli Haisch (Oxford University)
    09/08/2016, 15:30
  5. 14. Impact of astrophysical uncertainties on WIMP direct detection
    Prof. Anne Green (University of Nottingham)
    09/08/2016, 16:00
  6. 13. Quantifying compatibility among WIMP direct search data in a halo-independent way
    Ji-haeng Huh
    09/08/2016, 16:30
    We propose a novel halo-independent way of reporting the level of compatibility among WIMP direct search data sets. The main ingredient of the method is 'plausibility region', where any halo-function that can bring a certain level of compatibility should be fully contained in. The construction of the region is based on a new test statistic called "constrained parameter goodness-of-fit", which...
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  7. 15. Dark Matter Detectors and the Neutrino Wall
    Malcolm Fairbairn
    09/08/2016, 17:00
  8. 16. closeout/discussion
    09/08/2016, 17:30
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