A next-generation liquid xenon observatory for dark matter and neutrino physics

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doi:10.1088/1361-6471/ac841a

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, while featuring extensive sen- sitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.