The XENONnT Dark Matter Experiment
XENON Collaboration: E. Aprile, J. Aalbers, K. Abe, S. Ahmed Maouloud, L. Althueser, B. Andrieu, E. Angelino, J. R. Angevaare, V.C. Antochi, D. Ant\'on Martin, F. Arneodo, M. Balata, L. Baudis, A. L. Baxter, M. Bazyk, L. Bellagamba, R. Biondi, A. Bismark, E. J. Brookes, A. Brown

TL;DR
The XENONnT experiment is a large-scale liquid xenon detector designed to improve the sensitivity of dark matter detection, specifically WIMP particles, by reducing background noise and increasing target mass.
Contribution
This paper details the design, implementation, and initial performance results of the XENONnT detector, an upgrade over previous experiments to enhance dark matter search capabilities.
Findings
Extended sensitivity to WIMP dark matter by over an order of magnitude.
Successful operation of the detector with reduced background levels.
First science run results demonstrating detector performance.
Abstract
The multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter with two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in the program, planned to be an upgrade of its predecessor XENON1T. It features an active target of 5.9 tonnes of cryogenic liquid xenon (8.5 tonnes total mass in cryostat). The experiment is expected to extend the sensitivity to WIMP dark matter by more than an order of magnitude compared to XENON1T, thanks to the larger active mass and the significantly reduced background, improved by novel systems such as a radon removal plant and a neutron veto. This article describes the XENONnT experiment and its sub-systems in detail and reports on the detector performance during the first science run.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Scientific Research and Discoveries
