European Physical Journal C: Particles and Fields (Aug 2020)
Energy resolution and linearity of XENON1T in the MeV energy range
- E. Aprile,
- J. Aalbers,
- F. Agostini,
- M. Alfonsi,
- L. Althueser,
- F. D. Amaro,
- V. C. Antochi,
- E. Angelino,
- J. 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,
- M. Garbini,
- L. Grandi,
- 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 Xu,
- D. Wenz,
- C. Wittweg,
- J. Wulf,
- Z. Xu,
- M. Yamashita,
- J. Ye,
- G. Zavattini,
- Y. Zhang,
- T. Zhu,
- J. P. Zopounidis
Affiliations
- E. Aprile
- Physics Department, Columbia University
- J. Aalbers
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- F. Agostini
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- M. Alfonsi
- Institut für Physik & Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- L. Althueser
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- F. D. Amaro
- LIBPhys, Department of Physics, University of Coimbra
- V. C. Antochi
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- E. Angelino
- INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino
- J. Angevaare
- Nikhef and the University of Amsterdam
- F. Arneodo
- New York University Abu Dhabi
- D. Barge
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- L. Baudis
- Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute
- B. Bauermeister
- Department of Physics, Oskar Klein Centre, Stockholm University, AlbaNova
- 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 Zurich
- 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 Zurich
- J. M. R. Cardoso
- LIBPhys, Department of Physics, 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, AlbaNova
- 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
- INAF-Astrophysical Observatory of Torino, Department of Physics, 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 Zurich
- F. Gao
- Physics Department, Columbia University
- M. Garbini
- Department of Physics and Astronomy, University of Bologna and INFN-Bologna
- L. Grandi
- Department of Physics and Kavli Institute for Cosmological Physics, University of Chicago
- C. Hasterok
- Max-Planck-Institut für Kernphysik
- C. Hils
- Institut für Physik & Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- K. Hiraide
- Kamioka Observatory, Institute for Cosmic Ray Research, and 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, Nagoya University
- F. Joerg
- Max-Planck-Institut für Kernphysik
- N. Kato
- Kamioka Observatory, Institute for Cosmic Ray Research, and 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, 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
- LIBPhys, Department of Physics, University of Coimbra
- J. A. M. Lopes
- LIBPhys, Department of Physics, 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, AlbaNova
- L. Manenti
- Nikhef and the University of Amsterdam
- A. Manfredini
- Physik-Institut, University of Zurich
- F. Marignetti
- Department of Physics “Ettore Pancini”, University of Napoli and INFN-Napoli
- T. Marrodán Undagoitia
- Max-Planck-Institut für Kernphysik
- K. Martens
- Department of Physics and Kavli Institute for Cosmological Physics, University of Chicago
- 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, and 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 & 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, AlbaNova
- R. Peres
- Physik-Institut, University of Zurich
- J. Pienaar
- Department of Physics and 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 Zurich
- A. Rocchetti
- Physikalisches Institut, Universität Freiburg
- N. Rupp
- Max-Planck-Institut für Kernphysik
- J. M. F. dos Santos
- LIBPhys, Department of Physics, 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 & Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- S. Schindler
- Institut für Physik & 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 and Kavli Institute for Cosmological Physics, University of Chicago
- M. Silva
- LIBPhys, Department of Physics, University of Coimbra
- H. Simgen
- Max-Planck-Institut für Kernphysik
- A. Takeda
- Kamioka Observatory, Institute for Cosmic Ray Research, and 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
- INAF-Astrophysical Observatory of Torino, Department of Physics, 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 Zurich
- 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 Xu
- Department of Particle Physics and Astrophysics, Weizmann Institute of Science
- D. Wenz
- Institut für Physik & Exzellenzcluster PRISMA, Johannes Gutenberg-Universität Mainz
- C. Wittweg
- Institut für Kernphysik, Westfälische Wilhelms-Universität Münster
- J. Wulf
- Physik-Institut, University of Zurich
- Z. Xu
- Physics Department, Columbia University
- M. Yamashita
- Kamioka Observatory, Institute for Cosmic Ray Research, and 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
- INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- DOI
- https://doi.org/10.1140/epjc/s10052-020-8284-0
- Journal volume & issue
-
Vol. 80,
no. 8
pp. 1 – 9
Abstract
Abstract Xenon dual-phase time projection chambers designed to search for weakly interacting massive particles have so far shown a relative energy resolution which degrades with energy above $$\sim $$ ∼ 200 keV due to the saturation effects. This has limited their sensitivity in the search for rare events like the neutrinoless double-beta decay of $$^{136} \hbox {Xe}$$ 136Xe at its Q value, $$Q_{\beta \beta }\simeq 2.46\,\hbox {MeV}$$ Qββ≃2.46MeV . For the XENON1T dual-phase time projection chamber, we demonstrate that the relative energy resolution at $$1\,\sigma /\mu $$ 1σ/μ is as low as ($$0.80 \pm 0.02$$ 0.80±0.02 ) % in its one-ton fiducial mass, and for single-site interactions at $$Q_{\beta \beta }$$ Qββ . We also present a new signal correction method to rectify the saturation effects of the signal readout system, resulting in more accurate position reconstruction and indirectly improving the energy resolution. The very good result achieved in XENON1T opens up new windows for the xenon dual-phase dark matter detectors to simultaneously search for other rare events.