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Abstract
Two-phase noble liquid detectors, with large target masses and effective background reduction, are currently leading the dark matter direct detection for WIMP masses above a few GeV. Due to their sensitivity to single ionized electron signals, these detectors were shown to also have strong constraints for sub-GeV dark matter via their scattering on electrons. In fact, the most stringent direct detection constraints for sub-GeV dark matter down to as low as 5 MeV come from noble liquid detectors, namely XENON10, DarkSide-50, XENON100 and XENON1T, although these experiments still suffer from high background at single or a few electron level. LBECA is a planned 100-kg scale liquid xenon detector with significant reduction of the single and a few electron background. The experiment will improve the sensitivity to sub-GeV dark matter by three orders of magnitude compared to the current best constraints.
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Details
1 Lawrence Livermore National Laboratory (LLNL), Livermore, CA 94550-9698, USA
2 Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA
3 C.N. Yang Institute for Theoretical Physics, Stony Brook University, Stony Brook, NY 11794, USA
4 Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA
5 Department of Physics, University of California San Diego, La Jolla, CA 92093, USA
6 Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA 94720-8099, USA
7 C.N. Yang Institute for Theoretical Physics, Stony Brook University, Stony Brook, NY 11794, USA; Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA