Projected WIMP Sensitivity of the XENONnT Dark Matter Experiment
The XENON collaboration: E. Aprile, J. Aalbers, F. Agostini, M., Alfonsi, L. Althueser, F. D. Amaro, V. C. Antochi, E. Angelino, J. R., Angevaare, F. Arneodo, D. Barge, L. Baudis, B. Bauermeister, L. Bellagamba,, M. L. Benabderrahmane, T. Berger, A. Brown, E. Brown, S. Bruenner

TL;DR
The paper predicts XENONnT's ability to detect WIMPs, projecting sensitivity improvements over current limits and estimating background rates, with implications for dark matter detection.
Contribution
It provides detailed sensitivity projections and background estimates for XENONnT, including statistical methods ensuring proper coverage for future dark matter searches.
Findings
Projected sensitivity to WIMP-nucleon cross-section of 1.4×10⁻⁴⁸ cm² at 50 GeV/c²
Expected background rates of 12.3 and 2.2×10⁻³ (keV t y)⁻¹ for electronic and nuclear recoils
Discovery potential exceeds 3σ for cross-sections above 2.6×10⁻⁴⁸ cm²
Abstract
XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to (keV t y) and (keV t y), respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage. With the exposure goal of 20 ty, the expected sensitivity to spin-independent WIMP-nucleon interactions reaches a cross-section of cm for a 50…
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