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The XENONnT dark matter experiment.
Aprile, E; Aalbers, J; Abe, K; Ahmed Maouloud, S; Althueser, L; Andrieu, B; Angelino, E; Angevaare, J R; Antochi, V C; Antón Martin, D; Arneodo, F; Balata, M; Baudis, L; Baxter, A L; Bazyk, M; Bellagamba, L; Biondi, R; Bismark, A; Brookes, E J; Brown, A; Bruenner, S; Bruno, G; Budnik, R; Bui, T K; Cai, C; Cardoso, J M R; Cassese, F; Chiarini, A; Cichon, D; Cimental Chavez, A P; Colijn, A P; Conrad, J; Corrieri, R; Cuenca-García, J J; Cussonneau, J P; Dadoun, O; D'Andrea, V; Decowski, M P; De Fazio, B; Gangi, P Di; Diglio, S; Disdier, J M; Douillet, D; Eitel, K; Elykov, A; Farrell, S; Ferella, A D; Ferrari, C; Fischer, H; Flierman, M.
Afiliação
  • Aprile E; Physics Department, Columbia University, New York, NY 10027 USA.
  • Aalbers J; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Abe K; Kamioka Observatory, Institute for Cosmic Ray Research, and Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205 Japan.
  • Ahmed Maouloud S; LPNHE, Sorbonne Université, CNRS/IN2P3, 75005 Paris, France.
  • Althueser L; Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, 48149 Münster, Germany.
  • Andrieu B; LPNHE, Sorbonne Université, CNRS/IN2P3, 75005 Paris, France.
  • Angelino E; INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino, 10125 Turin, Italy.
  • Angevaare JR; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Antochi VC; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm, 10691 Sweden.
  • Antón Martin D; Department of Physics and Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637 USA.
  • Arneodo F; New York University Abu Dhabi-Center for Astro, Particle and Planetary Physics, Abu Dhabi, United Arab Emirates.
  • Balata M; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Baudis L; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Baxter AL; Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907 USA.
  • Bazyk M; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, 44307 Nantes, France.
  • Bellagamba L; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Biondi R; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Bismark A; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Brookes EJ; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Brown A; Physikalisches Institut, Universität Freiburg, 79104 Freiburg, Germany.
  • Bruenner S; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Bruno G; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, 44307 Nantes, France.
  • Budnik R; Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, 7610001 Israel.
  • Bui TK; Kamioka Observatory, Institute for Cosmic Ray Research, and Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205 Japan.
  • Cai C; Department of Physics and Center for High Energy Physics, Tsinghua University, Beijing, 100084 China.
  • Cardoso JMR; LIBPhys, Department of Physics, University of Coimbra, 3004-516 Coimbra, Portugal.
  • Cassese F; Department of Physics "Ettore Pancini", University of Napoli and INFN-Napoli, 80126 Naples, Italy.
  • Chiarini A; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Cichon D; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Cimental Chavez AP; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Colijn AP; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Conrad J; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm, 10691 Sweden.
  • Corrieri R; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Cuenca-García JJ; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Cussonneau JP; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, 44307 Nantes, France.
  • Dadoun O; LPNHE, Sorbonne Université, CNRS/IN2P3, 75005 Paris, France.
  • D'Andrea V; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Decowski MP; INFN-Roma Tre, 00146 Rome, Italy.
  • De Fazio B; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Gangi PD; Department of Physics "Ettore Pancini", University of Napoli and INFN-Napoli, 80126 Naples, Italy.
  • Diglio S; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Disdier JM; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, 44307 Nantes, France.
  • Douillet D; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Eitel K; IJCLab, CNRS/IN2P3, Université Paris-Saclay, Universit é de Paris, 15 rue Georges Clémenceau, 91400 Orsay, France.
  • Elykov A; Institute for Astroparticle Physics, Karlsruhe Institute of Technology, 76021 Karlsruhe, Germany.
  • Farrell S; Institute for Astroparticle Physics, Karlsruhe Institute of Technology, 76021 Karlsruhe, Germany.
  • Ferella AD; Department of Physics and Astronomy, Rice University, Houston, TX 77005 USA.
  • Ferrari C; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Fischer H; Department of Physics and Chemistry, University of L'Aquila, 67100 L'Aquila, Italy.
  • Flierman M; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
Eur Phys J C Part Fields ; 84(8): 784, 2024.
Article em En | MEDLINE | ID: mdl-39130092
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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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2024 Tipo de documento: Article País de publicação: França
Texto completo
Adicionar na Minha BVS
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2024 Tipo de documento: Article País de publicação: França