European Physical Journal C: Particles and Fields (Apr 2021)
$$^{222}$$ 222 Rn emanation measurements for the XENON1T experiment
- XENON Collaboration,
- E. Aprile,
- J. Aalbers,
- F. Agostini,
- M. Alfonsi,
- L. Althueser,
- F. D. Amaro,
- V. C. Antochi,
- E. Angelino,
- J. R. Angevaare,
- F. Arneodo,
- D. Barge,
- L. Baudis,
- B. Bauermeister,
- L. Bellagamba,
- M. L. Benabderrahmane,
- T. Berger,
- P. A. Breur,
- A. Brown,
- E. Brown,
- S. Bruenner,
- G. Bruno,
- R. Budnik,
- C. Capelli,
- J. M. R. Cardoso,
- D. Cichon,
- B. Cimmino,
- M. Clark,
- D. Coderre,
- A. P. Colijn,
- J. Conrad,
- J. P. Cussonneau,
- M. P. Decowski,
- A. Depoian,
- P. Di Gangi,
- A. Di Giovanni,
- R. Di Stefano,
- S. Diglio,
- A. Elykov,
- G. Eurin,
- A. D. Ferella,
- W. Fulgione,
- P. Gaemers,
- R. Gaior,
- A. Gallo Rosso,
- M. Galloway,
- F. Gao,
- L. Grandi,
- M. Garbini,
- C. Hasterok,
- C. Hils,
- K. Hiraide,
- L. Hoetzsch,
- E. Hogenbirk,
- J. Howlett,
- M. Iacovacci,
- Y. Itow,
- F. Joerg,
- N. Kato,
- S. Kazama,
- M. Kobayashi,
- G. Koltman,
- A. Kopec,
- H. Landsman,
- R. F. Lang,
- L. Levinson,
- Q. Lin,
- S. Lindemann,
- M. Lindner,
- F. Lombardi,
- J. A. M. Lopes,
- E. López Fune,
- C. Macolino,
- J. Mahlstedt,
- L. Manenti,
- A. Manfredini,
- F. Marignetti,
- T. Marrodán Undagoitia,
- K. Martens,
- J. Masbou,
- D. Masson,
- S. Mastroianni,
- M. Messina,
- K. Miuchi,
- A. Molinario,
- K. Morå,
- S. Moriyama,
- Y. Mosbacher,
- M. Murra,
- J. Naganoma,
- K. Ni,
- U. Oberlack,
- K. Odgers,
- J. Palacio,
- B. Pelssers,
- R. Peres,
- J. Pienaar,
- V. Pizzella,
- G. Plante,
- J. Qin,
- H. Qiu,
- D. Ramírez García,
- S. Reichard,
- A. Rocchetti,
- N. Rupp,
- J. M. F. dos Santos,
- G. Sartorelli,
- N. Šarčević,
- M. Scheibelhut,
- S. Schindler,
- J. Schreiner,
- D. Schulte,
- M. Schumann,
- L. Scotto Lavina,
- M. Selvi,
- F. Semeria,
- P. Shagin,
- E. Shockley,
- M. Silva,
- H. Simgen,
- A. Takeda,
- C. Therreau,
- D. Thers,
- F. Toschi,
- G. Trinchero,
- C. Tunnell,
- M. Vargas,
- G. Volta,
- O. Wack,
- H. Wang,
- Y. Wei,
- C. Weinheimer,
- M. Weiss,
- D. Wenz,
- J. Westermann,
- C. Wittweg,
- J. Wulf,
- Z. Xu,
- M. Yamashita,
- J. Ye,
- G. Zavattini,
- Y. Zhang,
- T. Zhu,
- J. P. Zopounidis
Affiliations
- XENON Collaboration
- Physics Department, Columbia University
- E. Aprile
- Physics Department, Columbia University
- J. Aalbers
- Department of Physics, Oskar Klein Centre, Stockholm University
- F. Agostini
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- M. Alfonsi
- Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- L. Althueser
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- F. D. Amaro
- Department of Physics, LIBPhys, University of Coimbra
- V. C. Antochi
- Department of Physics, Oskar Klein Centre, Stockholm University
- E. Angelino
- Department of Physics, INAF-Astrophysical Observatory of Torino, University of Torino and INFN-Torino
- J. R. Angevaare
- Nikhef and the University of Amsterdam
- F. Arneodo
- New York University Abu Dhabi
- D. Barge
- Department of Physics, Oskar Klein Centre, Stockholm University
- L. Baudis
- Physik-Institut, University of Zürich
- B. Bauermeister
- Department of Physics, Oskar Klein Centre, Stockholm University
- L. Bellagamba
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- M. L. Benabderrahmane
- New York University Abu Dhabi
- T. Berger
- Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute
- P. A. Breur
- Nikhef and the University of Amsterdam
- A. Brown
- Physik-Institut, University of Zürich
- E. Brown
- Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute
- S. Bruenner
- Nikhef and the University of Amsterdam
- G. Bruno
- New York University Abu Dhabi
- R. Budnik
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- C. Capelli
- Physik-Institut, University of Zürich
- J. M. R. Cardoso
- Department of Physics, LIBPhys, University of Coimbra
- D. Cichon
- Max-Planck-Institut für Kernphysik
- B. Cimmino
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- M. Clark
- Department of Physics and Astronomy, Purdue University
- D. Coderre
- Physikalisches Institut, Universität Freiburg
- A. P. Colijn
- Nikhef and the University of Amsterdam
- J. Conrad
- Department of Physics, Oskar Klein Centre, Stockholm University
- J. P. Cussonneau
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- M. P. Decowski
- Nikhef and the University of Amsterdam
- A. Depoian
- Department of Physics and Astronomy, Purdue University
- P. Di Gangi
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- A. Di Giovanni
- New York University Abu Dhabi
- R. Di Stefano
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- S. Diglio
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- A. Elykov
- Physikalisches Institut, Universität Freiburg
- G. Eurin
- Max-Planck-Institut für Kernphysik
- A. D. Ferella
- Department of Physics and Chemistry, University of L’Aquila
- W. Fulgione
- Department of Physics, INAF-Astrophysical Observatory of Torino, University of Torino and INFN-Torino
- P. Gaemers
- Nikhef and the University of Amsterdam
- R. Gaior
- LPNHE, Sorbonne Université, Université de Paris, CNRS/IN2P3
- A. Gallo Rosso
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- M. Galloway
- Physik-Institut, University of Zürich
- F. Gao
- Physics Department, Columbia University
- L. Grandi
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- M. Garbini
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- C. Hasterok
- Max-Planck-Institut für Kernphysik
- C. Hils
- Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- K. Hiraide
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo
- L. Hoetzsch
- Max-Planck-Institut für Kernphysik
- E. Hogenbirk
- Nikhef and the University of Amsterdam
- J. Howlett
- Physics Department, Columbia University
- M. Iacovacci
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- Y. Itow
- Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, and Institute for Space-Earth Environmental Research, Nagoya University
- F. Joerg
- Max-Planck-Institut für Kernphysik
- N. Kato
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo
- S. Kazama
- Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, and Institute for Space-Earth Environmental Research, Nagoya University
- M. Kobayashi
- Physics Department, Columbia University
- G. Koltman
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- A. Kopec
- Department of Physics and Astronomy, Purdue University
- H. Landsman
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- R. F. Lang
- Department of Physics and Astronomy, Purdue University
- L. Levinson
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- Q. Lin
- Physics Department, Columbia University
- S. Lindemann
- Physikalisches Institut, Universität Freiburg
- M. Lindner
- Max-Planck-Institut für Kernphysik
- F. Lombardi
- Department of Physics, LIBPhys, University of Coimbra
- J. A. M. Lopes
- Department of Physics, LIBPhys, University of Coimbra
- E. López Fune
- LPNHE, Sorbonne Université, Université de Paris, CNRS/IN2P3
- C. Macolino
- Université Paris-Saclay, CNRS/IN2P3, IJCLab
- J. Mahlstedt
- Department of Physics, Oskar Klein Centre, Stockholm University
- L. Manenti
- New York University Abu Dhabi
- A. Manfredini
- Physik-Institut, University of Zürich
- F. Marignetti
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- T. Marrodán Undagoitia
- Max-Planck-Institut für Kernphysik
- K. Martens
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo
- J. Masbou
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- D. Masson
- Physikalisches Institut, Universität Freiburg
- S. Mastroianni
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- M. Messina
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- K. Miuchi
- Department of Physics, Kobe University
- A. Molinario
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- K. Morå
- Physics Department, Columbia University
- S. Moriyama
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo
- Y. Mosbacher
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- M. Murra
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- J. Naganoma
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- K. Ni
- Department of Physics, University of California San Diego
- U. Oberlack
- Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- K. Odgers
- Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute
- J. Palacio
- Max-Planck-Institut für Kernphysik
- B. Pelssers
- Department of Physics, Oskar Klein Centre, Stockholm University
- R. Peres
- Physik-Institut, University of Zürich
- J. Pienaar
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- V. Pizzella
- Max-Planck-Institut für Kernphysik
- G. Plante
- Physics Department, Columbia University
- J. Qin
- Department of Physics and Astronomy, Purdue University
- H. Qiu
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- D. Ramírez García
- Physikalisches Institut, Universität Freiburg
- S. Reichard
- Physik-Institut, University of Zürich
- A. Rocchetti
- Department of Physics, University of California San Diego
- N. Rupp
- Max-Planck-Institut für Kernphysik
- J. M. F. dos Santos
- Department of Physics, LIBPhys, University of Coimbra
- G. Sartorelli
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- N. Šarčević
- Physikalisches Institut, Universität Freiburg
- M. Scheibelhut
- Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- S. Schindler
- Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- J. Schreiner
- Max-Planck-Institut für Kernphysik
- D. Schulte
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- M. Schumann
- Physikalisches Institut, Universität Freiburg
- L. Scotto Lavina
- LPNHE, Sorbonne Université, Université de Paris, CNRS/IN2P3
- M. Selvi
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- F. Semeria
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- P. Shagin
- Department of Physics and Astronomy, Rice University
- E. Shockley
- Department of Physics, Kavli Institute for Cosmological Physics, University of Chicago
- M. Silva
- Department of Physics, LIBPhys, University of Coimbra
- H. Simgen
- Max-Planck-Institut für Kernphysik
- A. Takeda
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo
- C. Therreau
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- D. Thers
- SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de Nantes
- F. Toschi
- Physikalisches Institut, Universität Freiburg
- G. Trinchero
- Department of Physics, INAF-Astrophysical Observatory of Torino, University of Torino and INFN-Torino
- C. Tunnell
- Department of Physics and Astronomy, Rice University
- M. Vargas
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- G. Volta
- Physik-Institut, University of Zürich
- O. Wack
- Max-Planck-Institut für Kernphysik
- H. Wang
- Physics and Astronomy Department, University of California
- Y. Wei
- Department of Physics, University of California San Diego
- C. Weinheimer
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- M. Weiss
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- D. Wenz
- Institut für Physik and Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- J. Westermann
- Max-Planck-Institut für Kernphysik
- C. Wittweg
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- J. Wulf
- Physik-Institut, University of Zürich
- Z. Xu
- Physics Department, Columbia University
- M. Yamashita
- Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo
- J. Ye
- Department of Physics, University of California San Diego
- G. Zavattini
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- Y. Zhang
- Physics Department, Columbia University
- T. Zhu
- Physics Department, Columbia University
- J. P. Zopounidis
- LPNHE, Sorbonne Université, Université de Paris, CNRS/IN2P3
- DOI
- https://doi.org/10.1140/epjc/s10052-020-08777-z
- Journal volume & issue
-
Vol. 81,
no. 4
pp. 1 – 14
Abstract
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 $$^{222}$$ 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 $$^{222}$$ 222 Rn activity concentration of $$10\,\mathrm{\,}\upmu \mathrm{Bq}/\mathrm{kg}$$ 10 μ Bq / kg in $$3.2\,\mathrm{t}$$ 3.2 t of xenon. The knowledge of the distribution of the $$^{222}$$ 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 $$^{222}$$ 222 Rn activity concentration in XENON1T. The final $$^{222}$$ 222 Rn activity concentration of $$(4.5\pm 0.1)\,\mathrm{\,}\upmu \mathrm{Bq}/\mathrm{kg}$$ ( 4.5 ± 0.1 ) μ Bq / kg in the target of XENON1T is the lowest ever achieved in a xenon dark matter experiment.