The XENON1T dark matter experiment

被引:0
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作者
E. Aprile
J. Aalbers
F. Agostini
M. Alfonsi
F. D. Amaro
M. Anthony
B. Antunes
F. Arneodo
M. Balata
P. Barrow
L. Baudis
B. Bauermeister
M. L. Benabderrahmane
T. Berger
A. Breskin
P. A. Breur
A. Brown
E. Brown
S. Bruenner
G. Bruno
R. Budnik
L. Bütikofer
J. Calvén
J. M. R. Cardoso
M. Cervantes
A. Chiarini
D. Cichon
D. Coderre
A. P. Colijn
J. Conrad
R. Corrieri
J. P. Cussonneau
M. P. Decowski
P. de Perio
P. Di Gangi
A. Di Giovanni
S. Diglio
J.-M. Disdier
M. Doets
E. Duchovni
G. Eurin
J. Fei
A. D. Ferella
A. Fieguth
D. Franco
D. Front
W. Fulgione
A. Gallo Rosso
M. Galloway
F. Gao
机构
[1] Laboratori Nazionli del Gran Sasso,Physics Department
[2] Columbia University,Department of Physics and Astrophysics
[3] Nikhef and the University of Amsterdam,Institut für Physik & Exzellenzcluster PRISMA
[4] INFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute,LIBPhys, Department of Physics
[5] University of Bologna and INFN-Bologna,Physik Institut
[6] Johannes Gutenberg-Universität Mainz,Oskar Klein Centre, Department of Physics
[7] University of Coimbra,Department of Physics, Applied Physics and Astronomy
[8] New York University Abu Dhabi,Department of Particle Physics and Astrophysics
[9] University of Zurich,Physikalisches Institut
[10] Stockholm University,Department of Physics and Astronomy
[11] AlbaNova,SUBATECH, IMT Atlantique
[12] Rensselaer Polytechnic Institute,Department of Physics
[13] Weizmann Institute of Science,Institut für Kernphysik
[14] Max-Planck-Institut für Kernphysik,Department of Physics and Kavli Institute of Cosmological Physics
[15] Universität Freiburg,Department of Physics and Astronomy
[16] Purdue University,LPNHE
[17] CNRS/IN2P3,Physics and Astronomy Department
[18] Université de Nantes,undefined
[19] University of California,undefined
[20] Westfälische Wilhelms-Universität Münster,undefined
[21] INFN-Torino and Osservatorio Astrofisico di Torino,undefined
[22] University of Chicago,undefined
[23] Rice University,undefined
[24] Université Pierre et Marie Curie,undefined
[25] Université Paris Diderot,undefined
[26] CNRS/IN2P3,undefined
[27] University of California,undefined
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摘要
The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2 t liquid xenon inventory, 2.0 t constitute the active target of the dual-phase time projection chamber. The scintillation and ionization signals from particle interactions are detected with low-background photomultipliers. This article describes the XENON1T instrument and its subsystems as well as strategies to achieve an unprecedented low background level. First results on the detector response and the performance of the subsystems are also presented.
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