Your browser doesn't support javascript.
loading
First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment.
Aprile, E; Abe, K; Agostini, F; Ahmed Maouloud, S; Althueser, L; Andrieu, B; Angelino, E; Angevaare, J R; Antochi, V C; Antón Martin, D; Arneodo, F; 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; Cichon, D; Cimental Chavez, A P; Colijn, A P; Conrad, J; Cuenca-García, J J; Cussonneau, J P; D'Andrea, V; Decowski, M P; Di Gangi, P; Di Pede, S; Diglio, S; Eitel, K; Elykov, A; Farrell, S; Ferella, A D; Ferrari, C; Fischer, H; Flierman, M; Fulgione, W; Fuselli, C; Gaemers, P; Gaior, R; Gallo Rosso, A; Galloway, M; Gao, F.
Afiliação
  • Aprile E; Physics Department, Columbia University, New York, New York 10027, USA.
  • 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.
  • Agostini F; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • 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 Torino, Italy.
  • Angevaare JR; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Antochi VC; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
  • Antón Martin D; Department of Physics and Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA.
  • Arneodo F; New York University Abu Dhabi-Center for Astro, Particle and Planetary Physics, Abu Dhabi, United Arab Emirates.
  • Baudis L; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Baxter AL; Department of Physics and Astronomy, Purdue University, West Lafayette, Indiana 47907, USA.
  • Bazyk M; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes 44307, 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, 1098XG Amsterdam, Netherlands.
  • Brown A; Physikalisches Institut, Universität Freiburg, 79104 Freiburg, Germany.
  • Bruenner S; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Bruno G; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes 44307, 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 & Center for High Energy Physics, Tsinghua University, Beijing 100084, China.
  • Cardoso JMR; LIBPhys, Department of Physics, University of Coimbra, 3004-516 Coimbra, Portugal.
  • 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, 1098XG Amsterdam, Netherlands.
  • Conrad J; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
  • Cuenca-García JJ; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Cussonneau JP; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes 44307, France.
  • D'Andrea V; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Decowski MP; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Di Gangi P; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Di Pede S; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Diglio S; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes 44307, France.
  • Eitel K; Institute for Astroparticle Physics, Karlsruhe Institute of Technology, 76021 Karlsruhe, Germany.
  • Elykov A; Institute for Astroparticle Physics, Karlsruhe Institute of Technology, 76021 Karlsruhe, Germany.
  • Farrell S; Department of Physics and Astronomy, Rice University, Houston, Texas 77005, USA.
  • Ferella AD; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Ferrari C; Department of Physics and Chemistry, University of L'Aquila, 67100 L'Aquila, Italy.
  • Fischer H; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Flierman M; Physikalisches Institut, Universität Freiburg, 79104 Freiburg, Germany.
  • Fulgione W; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Fuselli C; INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino, 10125 Torino, Italy.
  • Gaemers P; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Gaior R; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Gallo Rosso A; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Galloway M; LPNHE, Sorbonne Université, CNRS/IN2P3, 75005 Paris, France.
  • Gao F; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
Phys Rev Lett ; 131(4): 041003, 2023 Jul 28.
Article em En | MEDLINE | ID: mdl-37566859
ABSTRACT
We report on the first search for nuclear recoils from dark matter in the form of weakly interacting massive particles (WIMPs) with the XENONnT experiment, which is based on a two-phase time projection chamber with a sensitive liquid xenon mass of 5.9 ton. During the (1.09±0.03) ton yr exposure used for this search, the intrinsic ^{85}Kr and ^{222}Rn concentrations in the liquid target are reduced to unprecedentedly low levels, giving an electronic recoil background rate of (15.8±1.3) events/ton yr keV in the region of interest. A blind analysis of nuclear recoil events with energies between 3.3 and 60.5 keV finds no significant excess. This leads to a minimum upper limit on the spin-independent WIMP-nucleon cross section of 2.58×10^{-47} cm^{2} for a WIMP mass of 28 GeV/c^{2} at 90% confidence level. Limits for spin-dependent interactions are also provided. Both the limit and the sensitivity for the full range of WIMP masses analyzed here improve on previous results obtained with the XENON1T experiment for the same exposure.
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2023 Tipo de documento: Article País de afiliação: Estados Unidos
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2023 Tipo de documento: Article País de afiliação: Estados Unidos