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DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS

Journal Article · · European Physical Journal Plus
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  1. BATTELLE (PACIFIC NW LAB)
  2. Fondazione Bruno Kessler
  3. University of Houston
  4. Universidade de Sao Paulo
  5. Universita di Bologna
  6. Augustana College
  7. INFN-Bologna
  8. Politecnico di Milano
  9. CIEMAT Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
  10. Universita di Pisa
  11. INFN Milano Bicocca
  12. INFN Sezione di Pisa
  13. Universita Degli Studi Di Pisa
  14. Darkside collaboration
  15. Novosibirsk State University
  16. Laboratori Nazionali del Gran Sasso
  17. Carkside Collaboration
  18. Gran Sasso Science Institute
  19. Istituto Nazionale di Fisica Nucleare, Sezione di Genova
  20. Carleton University
  21. Universita degli Studi Roma Tre
  22. Budker Institute of Nuclear Physics
  23. Universita DI Cagliari
  24. INFN Genova Genova, Italy
  25. Institute for Particle Physics, ETH Zürich
  26. Darkside Collaboration
  27. Universita Degli Studi di Genova
  28. INFN Milano
  29. Universita degli Studi di Napoli Frederico II
  30. INFN, Sezione di Napoli
  31. INFN Napoli
  32. INFN - Genova
  33. Moscow State University
  34. INFN Bologna
  35. Universita Degli Studi di Sassari
  36. INFN Torino
  37. CIEMATCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas
  38. INFN
  39. Universite de Paris VI (Pierre et Marie Curie)
  40. Saint Petersburg Nuclear Physics Institute
  41. Princeton University
  42. National Institute for R&D of Isotopic and Molecular Technologies
  43. Joint Institute for Nuclear Research
  44. Universite de Paris VII (Denis Diderot)
  45. University of Crete
  46. INFN Milano, Milano, Italy
  47. CIEMAT
  48. Institute for Particle Physics
  49. Triumf
  50. Temple University
  51. INFN Pisa
  52. National Research Centre Kurchatov Institute
  53. Institute of High Energy Physics
  54. Black Hills State University
  55. INFN Laboratori Nazionali del Sud
  56. Fort Lewis College
  57. Queen's University (Ontario)
  58. INFN Cagliari
  59. Laurentian University of Sudbury
  60. University of California, Davis
  61. Fermi National Accelerator Laboratory,
  62. Belgorod National Research University
  63. University of Alberta
  64. INFN Sezione di Roma
  65. Universidade Estadual de Campinas
  66. Universita Degli Studi Di Trento
  67. University of Hawaii
  68. University of London
  69. University of Massachusetts at Amherst
  70. ETH Zurich
  71. Physics Department, Universit degli Studi - Genova
  72. INFN Bologna, Italy
  73. Radiation Physics Laboratory, Belgorod National Research University
  74. Budker Institute of Nuclear Physics, Russia
  75. National Research Centre Kurchatov Institute, Rusia
  76. Radiaition Physics Laboratory, Belgorod University
  77. Universit degli Studi and INFN, 16146 Genova, Italy
  78. INFN, Laboratori Nazionali del Gran Sasso, Assergi, Italy
  79. Fondazione Bruno Kessler, Povo 38123, Italy
  80. Lomonosov Moscow State University
  81. University of Sussex
  82. Uniwersytet Jagiellonski
  83. INFN Pisa, Pisa, Italy
  84. Universita degli Studi di Perugia
  85. INFN Laboratori Nazionali del Gran Sasso, Italy
  86. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
  87. INFN Pisa, Italy
  88. Universita degli studi di Milano
  89. INFN- Cagliari
  90. University of California, Los Angeles
  91. INFN Gran Sasso
  92. TRIUMF
  93. Fermi National Accelerator Laboratory
  94. National Research Centre, Kurchatov Institute, Russia
  95. Joint Institute for Nuclear Research, Russia
  96. INFN Genova
  97. INFN Laboratori Nazionali del Sud, Italy
  98. Laboratori Nazionali del Gran Sasso, Italy
  99. Universita Degli Studi, Cagliari, Italy
  100. SNOLAB
  101. Universita Degli Studi di Roma La Sapienza
  102. Joint Institute for Nuclear Research, Dubna, Russia
  103. Virginia Polytechnic Institute
  104. Harvard University
  105. Institute of High Energy Physics CAS, China
  106. CIEMAT, Madrid, Spain
  107. INFN Milano, Italy
  108. INFN Sezione di Roma, Italy

Abstract. Building on the successful experience in operating the DarkSide-50 detector, the DarkSide Collaboration is going to construct DarkSide-20k, a direct WIMP search detector using a two-phase Liquid Argon Time Projection Chamber (LAr TPC) with an active (fiducial) mass of 23 t (20 t). This paper describes a preliminary design for the experiment, in which the DarkSide-20k LAr TPC is deployed within a shield/veto with a spherical Liquid Scintillator Veto (LSV) inside a cylindrical Water Cherenkov Veto (WCV). This preliminary design provides a baseline for the experiment to achieve its physics goals, while further development work will lead to the final optimization of the detector parameters and an eventual technical design. Operation of DarkSide-50 demonstrated a major reduction in the dominant 39Ar background when using argon extracted from an underground source, before applying pulse shape analysis. Data from DarkSide-50, in combination with MC simulation and analytical modeling, shows that a rejection factor for discrimination between electron and nuclear recoils of > 3 × 109 is achievable. This, along with the use of the veto system and utilizing silicon photomultipliers in the LAr TPC, are the keys to unlocking the path to large LAr TPC detector masses, while maintaining an experiment in which less than < 0.1 events (other than ?-induced nuclear recoils) is expected to occur within the WIMP search region during the planned exposure. DarkSide-20k will have ultra-low backgrounds than can be measured in situ, giving sensitivity to WIMP-nucleon cross sections of 1.2×10 -47 cm2 (1.1×10 -46 cm2) for WIMPs of 1TeV/c2 (10TeV/c2) mass, to be achieved during a 5 yr run producing an exposure of 100 t yr free from any instrumental background.

Research Organization:
Pacific Northwest National Laboratory (PNNL), Richland, WA (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
AC05-76RL01830
OSTI ID:
1719103
Report Number(s):
PNNL-SA-134133
Journal Information:
European Physical Journal Plus, Vol. 133, Issue 3
Country of Publication:
United States
Language:
English

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Silicon Photomultipliers: Technology Optimizations for Ultraviolet, Visible and Near-Infrared Range February 2019
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$Z'$ Mediated WIMPs: Dead, Dying, or Soon to be Detected? January 2019

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