Abstract

A low-energy electronic recoil calibration of XENON1T, a dual-phase xenon time projection chamber, with an internal 37Ar source was performed. This calibration source features a 35-day half-life and provides two mono-energetic lines at 2.82 keV and 0.27 keV. The photon yield and electron yield at 2.82 keV are measured to be (32.3±0.3) photons/keV and (40.6±0.5) electrons/keV, respectively, in agreement with other measurements and with NEST predictions. The electron yield at 0.27 keV is also measured and it is (68.0-3.7+6.3) electrons/keV. The 37Ar calibration confirms that the detector is well-understood in the energy region close to the detection threshold, with the 2.82 keV line reconstructed at (2.83±0.02) keV, which further validates the model used to interpret the low-energy electronic recoil excess previously reported by XENON1T. The ability to efficiently remove argon with cryogenic distillation after the calibration proves that 37Ar can be considered as a regular calibration source for multi-tonne xenon detectors.

Details

Title
Low-energy calibration of XENON1T with an internal 37Ar source
Author
Aprile, E. 1 ; Abe, K. 2 ; Agostini, F. 3 ; Ahmed Maouloud, S. 4 ; Alfonsi, M. 5 ; Althueser, L. 6 ; Andrieu, B. 4 ; Angelino, E. 7 ; Angevaare, J. R. 8 ; Antochi, V. C. 9 ; Antón Martin, D. 10 ; Arneodo, F. 11 ; Baudis, L. 12 ; Baxter, A. L. 13 ; Bellagamba, L. 3 ; Biondi, R. 14 ; Bismark, A. 12 ; Brown, A. 15 ; Bruenner, S. 8 ; Bruno, G. 16 ; Budnik, R. 17 ; Bui, T. K. 2 ; Cai, C. 18 ; Capelli, C. 12 ; Cardoso, J. M. R. 19 ; Cichon, D. 20 ; Colijn, A. P. 8 ; Conrad, J. 9 ; Cuenca-García, J. J. 21 ; Cussonneau, J. P. 16 ; D’Andrea, V. 22 ; Decowski, M. P. 8 ; Di Gangi, P. 3 ; Di Pede, S. 8 ; Diglio, S. 16 ; Eitel, K. 23 ; Elykov, A. 15 ; Farrell, S. 24 ; Ferella, A. D. 25 ; Ferrari, C. 26 ; Fischer, H. 15 ; Fulgione, W. 27 ; Gaemers, P. 8 ; Gaior, R. 4 ; Gallo Rosso, A. 9 ; Galloway, M. 12 ; Gao, F. 18 ; Glade-Beucke, R. 15 ; Grandi, L. 10 ; Grigat, J. 15 ; Guida, M. 20 ; Hammann, R. 20 ; Higuera, A. 24 ; Hils, C. 5 ; Hoetzsch, L. 20 ; Howlett, J. 1 ; Iacovacci, M. 28 ; Itow, Y. 29 ; Jakob, J. 6 ; Joerg, F. 20 ; Joy, A. 9 ; Kato, N. 2 ; Kara, M. 23 ; Kavrigin, P. 17 ; Kazama, S. 29 ; Kobayashi, M. 29 ; Koltman, G. 17 ; Kopec, A. 30 ; Kuger, F. 15 ; Landsman, H. 17 ; Lang, R. F. 13 ; Levinson, L. 17 ; Li, I. 24 ; Li, S. 13 ; Liang, S. 24 ; Lindemann, S. 15 ; Lindner, M. 20 ; Liu, K. 18 ; Loizeau, J. 16 ; Lombardi, F. 5 ; Long, J. 10 ; Lopes, J. A. M. 31 ; Ma, Y. 30 ; Macolino, C. 25 ; Mahlstedt, J. 9 ; Mancuso, A. 3 ; Manenti, L. 11 ; Marignetti, F. 28 ; Marrodán Undagoitia, T. 20 ; Martens, K. 2 ; Masbou, J. 16 ; Masson, D. 15 ; Masson, E. 4 ; Mastroianni, S. 28 ; Messina, M. 26 ; Miuchi, K. 32 ; Mizukoshi, K. 32 ; Molinario, A. 7 ; Moriyama, S. 2 ; Morå, K. 1 ; Mosbacher, Y. 17 ; Murra, M. 1 ; Müller, J. 15 ; Ni, K. 30 ; Oberlack, U. 5 ; Paetsch, B. 17 ; Palacio, J. 20 ; Peres, R. 12 ; Peters, C. 24 ; Pienaar, J. 10 ; Pierre, M. 16 ; Pizzella, V. 20 ; Plante, G. 1 ; Qi, J. 30 ; Qin, J. 13 ; Ramírez García, D. 12 ; Reichard, S. 23 ; Rocchetti, A. 15 ; Rupp, N. 20 ; Sanchez, L. 24 ; Sanchez-Lucas, P. 12 ; Santos, J. M. F. dos 19 ; Sarnoff, I. 11 ; Sartorelli, G. 3 ; Schreiner, J. 20 ; Schulte, D. 6 ; Schulte, P. 6 ; Schulze Eißing, H. 6 ; Schumann, M. 15 ; Lavina, L. Scotto 4 ; Selvi, M. 3 ; Semeria, F. 3 ; Shagin, P. 5 ; Shi, S. 1 ; Shockley, E. 30 ; Silva, M. 19 ; Simgen, H. 20 ; Takeda, A. 2 ; Tan, P.-L. 9 ; Terliuk, A. 33 ; Thers, D. 16 ; Toschi, F. 15 ; Trinchero, G. 7 ; Tunnell, C. 24 ; Tönnies, F. 15 ; Valerius, K. 23 ; Volta, G. 12 ; Weinheimer, C. 6 ; Weiss, M. 17 ; Wenz, D. 5 ; Wittweg, C. 12 ; Wolf, T. 20 ; Xu, D. 1 ; Xu, Z. 1 ; Yamashita, M. 2 ; Yang, L. 30 ; Ye, J. 1 ; Yuan, L. 10 ; Zavattini, G. 34 ; Zerbo, S. 1 ; Zhong, M. 30 ; Zhu, T. 1 ; Geppert, C. 35 ; Riemer, J. 35 

 Columbia University, Physics Department, New York, USA (GRID:grid.21729.3f) (ISNI:0000000419368729) 
 University of Tokyo, Kamioka Observatory, Institute for Cosmic Ray Research, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Hida, Japan (GRID:grid.26999.3d) (ISNI:0000 0001 2151 536X) 
 University of Bologna and INFN-Bologna, Department of Physics and Astronomy, Bologna, Italy (GRID:grid.6292.f) (ISNI:0000 0004 1757 1758) 
 LPNHE, Sorbonne Université, CNRS/IN2P3, Paris, France (GRID:grid.463935.e) (ISNI:0000 0000 9463 7096) 
 Johannes Gutenberg-Universität Mainz, Institut für Physik & Exzellenzcluster PRISMA+, Mainz, Germany (GRID:grid.5802.f) (ISNI:0000 0001 1941 7111) 
 Westfälische Wilhelms-Universität Münster, Institut für Kernphysik, Münster, Germany (GRID:grid.5949.1) (ISNI:0000 0001 2172 9288) 
 INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino, Turin, Italy (GRID:grid.436940.c) 
 Nikhef and the University of Amsterdam, Amsterdam, The Netherlands (GRID:grid.7177.6) (ISNI:0000000084992262) 
 Stockholm University, AlbaNova, Department of Physics, Oskar Klein Centre, Stockholm, Sweden (GRID:grid.10548.38) (ISNI:0000 0004 1936 9377) 
10  University of Chicago, Department of Physics, Kavli Institute for Cosmological Physics, Chicago, USA (GRID:grid.170205.1) (ISNI:0000 0004 1936 7822) 
11  New York University Abu Dhabi, Center for Astro, Particle and Planetary Physics, Abu Dhabi, United Arab Emirates (GRID:grid.440573.1) (ISNI:0000 0004 1755 5934) 
12  University of Zürich, Physik-Institut, Zurich, Switzerland (GRID:grid.7400.3) (ISNI:0000 0004 1937 0650) 
13  Purdue University, Department of Physics and Astronomy, West Lafayette, USA (GRID:grid.169077.e) (ISNI:0000 0004 1937 2197) 
14  INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466877.c) (ISNI:0000 0001 2201 8832); Max-Planck-Institut für Kernphysik, Heidelberg, Germany (GRID:grid.419604.e) (ISNI:0000 0001 2288 6103) 
15  Universität Freiburg, Physikalisches Institut, Freiburg, Germany (GRID:grid.5963.9) 
16  Université de Nantes, SUBATECH, IMT Atlantique, CNRS/IN2P3, Nantes, France (GRID:grid.4817.a) (ISNI:0000 0001 2189 0784) 
17  Weizmann Institute of Science, Department of Particle Physics and Astrophysics, Rehovot, Israel (GRID:grid.13992.30) (ISNI:0000 0004 0604 7563) 
18  Tsinghua University, Department of Physics, Center for High Energy Physics, Beijing, China (GRID:grid.12527.33) (ISNI:0000 0001 0662 3178) 
19  University of Coimbra, LIBPhys, Department of Physics, Coimbra, Portugal (GRID:grid.8051.c) (ISNI:0000 0000 9511 4342) 
20  Max-Planck-Institut für Kernphysik, Heidelberg, Germany (GRID:grid.419604.e) (ISNI:0000 0001 2288 6103) 
21  University of Zürich, Physik-Institut, Zurich, Switzerland (GRID:grid.7400.3) (ISNI:0000 0004 1937 0650); Karlsruhe Institute of Technology, Institute for Astroparticle Physics, Karlsruhe, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874) 
22  INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466877.c) (ISNI:0000 0001 2201 8832); Universität Freiburg, Physikalisches Institut, Freiburg, Germany (GRID:grid.5963.9); University of L’Aquila, Department of Physics and Chemistry, L’Aquila, Italy (GRID:grid.158820.6) (ISNI:0000 0004 1757 2611) 
23  Karlsruhe Institute of Technology, Institute for Astroparticle Physics, Karlsruhe, Germany (GRID:grid.7892.4) (ISNI:0000 0001 0075 5874) 
24  Rice University, Department of Physics and Astronomy, Houston, USA (GRID:grid.21940.3e) (ISNI:0000 0004 1936 8278) 
25  INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466877.c) (ISNI:0000 0001 2201 8832); University of L’Aquila, Department of Physics and Chemistry, L’Aquila, Italy (GRID:grid.158820.6) (ISNI:0000 0004 1757 2611) 
26  INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466877.c) (ISNI:0000 0001 2201 8832) 
27  INAF-Astrophysical Observatory of Torino, Department of Physics, University of Torino and INFN-Torino, Turin, Italy (GRID:grid.436940.c); INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, L’Aquila, Italy (GRID:grid.466877.c) (ISNI:0000 0001 2201 8832) 
28  University of Napoli and INFN-Napoli, Department of Physics “Ettore Pancini”, Naples, Italy (GRID:grid.4691.a) (ISNI:0000 0001 0790 385X) 
29  Nagoya University, Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Institute for Space-Earth Environmental Research, Nagoya, Japan (GRID:grid.27476.30) (ISNI:0000 0001 0943 978X) 
30  University of California San Diego, Department of Physics, La Jolla, USA (GRID:grid.266100.3) (ISNI:0000 0001 2107 4242) 
31  University of Coimbra, LIBPhys, Department of Physics, Coimbra, Portugal (GRID:grid.8051.c) (ISNI:0000 0000 9511 4342); Coimbra Polytechnic - ISEC, Coimbra, Portugal (GRID:grid.8051.c) 
32  Kobe University, Department of Physics, Kobe, Japan (GRID:grid.31432.37) (ISNI:0000 0001 1092 3077) 
33  Max-Planck-Institut für Kernphysik, Heidelberg, Germany (GRID:grid.419604.e) (ISNI:0000 0001 2288 6103); Universität Heidelberg, Physikalisches Institut, Heidelberg, Germany (GRID:grid.7700.0) (ISNI:0000 0001 2190 4373) 
34  University of Bologna and INFN-Bologna, Department of Physics and Astronomy, Bologna, Italy (GRID:grid.6292.f) (ISNI:0000 0004 1757 1758); Università di Ferrara, INFN, Sez. di Ferrara and Dip. di Fisica e Scienze della Terra, Ferrara (FE), Italy (GRID:grid.8484.0) (ISNI:0000 0004 1757 2064) 
35  Johannes Gutenberg-Universität Mainz, Forschungsreaktor TRIGA Mainz, Mainz, Germany (GRID:grid.5802.f) (ISNI:0000 0001 1941 7111) 
Pages
542
Publication year
2023
Publication date
Jun 2023
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2829977880
Copyright
© The Author(s) 2023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.