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![Per-nucleon spin-independent scattering cross sections and dark matter masses that can be probed by liquid xenon dark matter detectors via dedicated searches for multi-scatter signals. For cross sections above σMIMP (horizontal green lines) one expects dark matter to scatter multiple times in the detector while transiting. The maximum mass reachable (vertical green lines) is limited by the total integrated flux of dark matter in the detector over the runtime of the experiment. Masses up to and beyond the Planck mass 10 19 GeV/c 2 may be probed with a next-generation detector. Only smaller cross-sections and smaller masses are probed by the standard single-scatter analyses (blue lines). Figure taken from Ref. [141].](publication/359054301/figure/fig14/AS:1130869616050179@1646631735105/Per-nucleon-spin-independent-scattering-cross-sections-and-dark-matter-masses-that-can-be.png)
Per-nucleon spin-independent scattering cross sections and dark matter masses that can be probed by liquid xenon dark matter detectors via dedicated searches for multi-scatter signals. For cross sections above σMIMP (horizontal green lines) one expects dark matter to scatter multiple times in the detector while transiting. The maximum mass reachable (vertical green lines) is limited by the total integrated flux of dark matter in the detector over the runtime of the experiment. Masses up to and beyond the Planck mass 10 19 GeV/c 2 may be probed with a next-generation detector. Only smaller cross-sections and smaller masses are probed by the standard single-scatter analyses (blue lines). Figure taken from Ref. [141].
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The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for Weakly Interacting Massive Particles (WIMPs), while featuring extensive sensitivity to many alternative dark matt...
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