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Light Dark Matter Search with Ionization Signals in XENON1T.
Aprile, E; Aalbers, J; Agostini, F; Alfonsi, M; Althueser, L; Amaro, F D; Antochi, V C; Angelino, E; Arneodo, F; Barge, D; Baudis, L; Bauermeister, B; Bellagamba, L; Benabderrahmane, M L; Berger, T; Breur, P A; Brown, A; Brown, E; Bruenner, S; Bruno, G; Budnik, R; Capelli, C; Cardoso, J M R; Cichon, D; Coderre, D; Colijn, A P; Conrad, J; Cussonneau, J P; Decowski, M P; de Perio, P; Depoian, A; Di Gangi, P; Di Giovanni, A; Diglio, S; Elykov, A; Eurin, G; Fei, J; Ferella, A D; Fieguth, A; Fulgione, W; Gaemers, P; Gallo Rosso, A; Galloway, M; Gao, F; Garbini, M; Grandi, L; Greene, Z; Hasterok, C; Hils, C; Hogenbirk, E.
Afiliação
  • Aprile E; Physics Department, Columbia University, New York, New York 10027, USA.
  • Aalbers J; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
  • Agostini F; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Alfonsi M; Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany.
  • Althueser L; Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, 48149 Münster, Germany.
  • Amaro FD; LIBPhys, Department of Physics, University of Coimbra, 3004-516 Coimbra, Portugal.
  • Antochi VC; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
  • Angelino E; INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino, 10125 Torino, Italy.
  • Arneodo F; New York University Abu Dhabi, PO Box 129188, Abu Dhabi, United Arab Emirates.
  • Barge D; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
  • Baudis L; Physik-Institut, University of Zurich, 8057 Zurich, Switzerland.
  • Bauermeister B; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
  • Bellagamba L; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Benabderrahmane ML; New York University Abu Dhabi, PO Box 129188, Abu Dhabi, United Arab Emirates.
  • Berger T; Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, Troy, New York 12180, USA.
  • Breur PA; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Brown A; Physik-Institut, University of Zurich, 8057 Zurich, Switzerland.
  • Brown E; Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, Troy, New York 12180, USA.
  • Bruenner S; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Bruno G; New York University Abu Dhabi, PO Box 129188, Abu Dhabi, United Arab Emirates.
  • Budnik R; Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel.
  • Capelli C; Physik-Institut, University of Zurich, 8057 Zurich, Switzerland.
  • Cardoso JMR; LIBPhys, Department of Physics, University of Coimbra, 3004-516 Coimbra, Portugal.
  • Cichon D; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Coderre D; Physikalisches Institut, Universität Freiburg, 79104 Freiburg, Germany.
  • 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.
  • Cussonneau JP; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes 44307, France.
  • Decowski MP; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • de Perio P; Physics Department, Columbia University, New York, New York 10027, USA.
  • Depoian A; Department of Physics and Astronomy, Purdue University, West Lafayette, Indiana 47907, USA.
  • Di Gangi P; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Di Giovanni A; New York University Abu Dhabi, PO Box 129188, Abu Dhabi, United Arab Emirates.
  • Diglio S; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, Nantes 44307, France.
  • Elykov A; Physikalisches Institut, Universität Freiburg, 79104 Freiburg, Germany.
  • Eurin G; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Fei J; Department of Physics, University of California, San Diego, California 92093, USA.
  • Ferella AD; Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, Stockholm SE-10691, Sweden.
  • Fieguth A; Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, 48149 Münster, Germany.
  • Fulgione W; 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.
  • Gallo Rosso A; Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, Netherlands.
  • Galloway M; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Gao F; Physik-Institut, University of Zurich, 8057 Zurich, Switzerland.
  • Garbini M; Physics Department, Columbia University, New York, New York 10027, USA.
  • Grandi L; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Greene Z; Department of Physics and Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA.
  • Hasterok C; Physics Department, Columbia University, New York, New York 10027, USA.
  • Hils C; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Hogenbirk E; Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany.
Phys Rev Lett ; 123(25): 251801, 2019 Dec 20.
Article em En | MEDLINE | ID: mdl-31922764
ABSTRACT
We report constraints on light dark matter (DM) models using ionization signals in the XENON1T experiment. We mitigate backgrounds with strong event selections, rather than requiring a scintillation signal, leaving an effective exposure of (22±3) tonne day. Above ∼0.4 keV_{ee}, we observe <1 event/(tonne day keV_{ee}), which is more than 1000 times lower than in similar searches with other detectors. Despite observing a higher rate at lower energies, no DM or CEvNS detection may be claimed because we cannot model all of our backgrounds. We thus exclude new regions in the parameter spaces for DM-nucleus scattering for DM masses m_{χ} within 3-6 GeV/c^{2}, DM-electron scattering for m_{χ}>30 MeV/c^{2}, and absorption of dark photons and axionlike particles for m_{χ} within 0.186-1 keV/c^{2}.
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2019 Tipo de documento: Article País de afiliação: Estados Unidos
Texto completo
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2019 Tipo de documento: Article País de afiliação: Estados Unidos