K. Morå

TL;DR: In this article, the XENON1T data was used for searches for new physics with low-energy electronic recoil data recorded with the Xenon1T detector, which enabled one of the most sensitive searches for solar axions, an enhanced neutrino magnetic moment using solar neutrinos, and bosonic dark matter.

TL;DR: The DARWIN detector as mentioned in this paper is an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core, whose primary goal is to explore the experimentally accessible parameter space for Weakly Interacting Massive Particles (WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background.

TL;DR: In this paper, the authors predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs) in a 4 t fiducial mass.

TL;DR: In this article, the authors predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs) using the profile construction method, in order to ensure proper coverage.

TL;DR: In this article, the authors report results from searches for new physics with low-energy electronic recoil data recorded with the XENON1T detector, with an exposure of 065 t-y and an unprecedentedly low background rate of $76 \pm 2-stat}$ events/(t y keV) between 1-30 keV.