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222 Rn  emanation measurements for the XENON1T experiment.
Aprile, E; Aalbers, J; Agostini, F; Alfonsi, M; Althueser, L; Amaro, F D; Antochi, V C; Angelino, E; Angevaare, J R; 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; Cimmino, B; Clark, M; Coderre, D; Colijn, A P; Conrad, J; Cussonneau, J P; Decowski, M P; Depoian, A; Di Gangi, P; Di Giovanni, A; Di Stefano, R; Diglio, S; Elykov, A; Eurin, G; Ferella, A D; Fulgione, W; Gaemers, P; Gaior, R; Rosso, A Gallo; Galloway, M; Gao, F; Grandi, L; Garbini, M; Hasterok, C; Hils, C.
Afiliação
  • Aprile E; Physics Department, Columbia University, New York, NY 10027 USA.
  • Aalbers J; Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova, 10691 Stockholm, 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; Department of Physics, LIBPhys, University of Coimbra, 3004-516 Coimbra, Portugal.
  • Antochi VC; Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova, 10691 Stockholm, Sweden.
  • Angelino E; Department of Physics, INAF-Astrophysical Observatory of Torino, University of Torino and INFN-Torino, 10125 Turin, Italy.
  • Angevaare JR; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Arneodo F; New York University Abu Dhabi, Abu Dhabi, United Arab Emirates.
  • Barge D; Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova, 10691 Stockholm, Sweden.
  • Baudis L; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Bauermeister B; Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova, 10691 Stockholm, Sweden.
  • Bellagamba L; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Benabderrahmane ML; New York University Abu Dhabi, Abu Dhabi, United Arab Emirates.
  • Berger T; Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, Troy, NY 12180 USA.
  • Breur PA; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Brown A; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Brown E; Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, Troy, NY 12180 USA.
  • Bruenner S; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Bruno G; New York University Abu Dhabi, Abu Dhabi, United Arab Emirates.
  • Budnik R; Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, 7610001 Israel.
  • Capelli C; Simons Center for Geometry and Physics and C. N. Yang Institute for Theoretical Physics, SUNY, Stony Brook, NY USA.
  • Cardoso JMR; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Cichon D; Department of Physics, LIBPhys, University of Coimbra, 3004-516 Coimbra, Portugal.
  • Cimmino B; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Clark M; Department of Physics "Ettore Pancini", University of Napoli and INFN-Napoli, 80126 Naples, Italy.
  • Coderre D; Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907 USA.
  • Colijn AP; Physikalisches Institut, Universität Freiburg, 79104 Freiburg, Germany.
  • Conrad J; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Cussonneau JP; Institute for Subatomic Physics, Utrecht University, Utrecht, Netherlands.
  • Decowski MP; Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova, 10691 Stockholm, Sweden.
  • Depoian A; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, 44307 Nantes, France.
  • Di Gangi P; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Di Giovanni A; Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907 USA.
  • Di Stefano R; Department of Physics and Astronomy, University of Bologna and INFN-Bologna, 40126 Bologna, Italy.
  • Diglio S; New York University Abu Dhabi, Abu Dhabi, United Arab Emirates.
  • Elykov A; Department of Physics "Ettore Pancini", University of Napoli and INFN-Napoli, 80126 Naples, Italy.
  • Eurin G; SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes, 44307 Nantes, France.
  • Ferella AD; Physikalisches Institut, Universität Freiburg, 79104 Freiburg, Germany.
  • Fulgione W; Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany.
  • Gaemers P; Department of Physics and Chemistry, University of L'Aquila, 67100 L'Aquila, Italy.
  • Gaior R; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Rosso AG; Department of Physics, INAF-Astrophysical Observatory of Torino, University of Torino and INFN-Torino, 10125 Turin, Italy.
  • Galloway M; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Gao F; Nikhef and the University of Amsterdam, Science Park, 1098 XG Amsterdam, The Netherlands.
  • Grandi L; LPNHE, Sorbonne Université, Université de Paris, CNRS/IN2P3, Paris, France.
  • Garbini M; INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Hasterok C; Physik-Institut, University of Zürich, 8057 Zürich, Switzerland.
  • Hils C; Physics Department, Columbia University, New York, NY 10027 USA.
Eur Phys J C Part Fields ; 81(4): 337, 2021.
Article em En | MEDLINE | ID: mdl-34720714
ABSTRACT
The selection of low-radioactive construction materials is of utmost importance for the success of low-energy rare event search experiments. Besides radioactive contaminants in the bulk, the emanation of radioactive radon atoms from material surfaces attains increasing relevance in the effort to further reduce the background of such experiments. In this work, we present the 222 Rn emanation measurements performed for the XENON1T dark matter experiment. Together with the bulk impurity screening campaign, the results enabled us to select the radio-purest construction materials, targeting a 222 Rn activity concentration of 10 µ Bq / kg in 3.2 t of xenon. The knowledge of the distribution of the 222 Rn sources allowed us to selectively eliminate problematic components in the course of the experiment. The predictions from the emanation measurements were compared to data of the 222 Rn activity concentration in XENON1T. The final 222 Rn activity concentration of ( 4.5 ± 0.1 ) µ Bq / kg in the target of XENON1T is the lowest ever achieved in a xenon dark matter experiment.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2021 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2021 Tipo de documento: Article