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First Results from the DEAP-3600 Dark Matter Search with Argon at SNOLAB.
Amaudruz, P-A; Baldwin, M; Batygov, M; Beltran, B; Bina, C E; Bishop, D; Bonatt, J; Boorman, G; Boulay, M G; Broerman, B; Bromwich, T; Bueno, J F; Burghardt, P M; Butcher, A; Cai, B; Chan, S; Chen, M; Chouinard, R; Cleveland, B T; Cranshaw, D; Dering, K; DiGioseffo, J; Dittmeier, S; Duncan, F A; Dunford, M; Erlandson, A; Fatemighomi, N; Florian, S; Flower, A; Ford, R J; Gagnon, R; Giampa, P; Golovko, V V; Gorel, P; Gornea, R; Grace, E; Graham, K; Gulyev, E; Hakobyan, R; Hall, A; Hallin, A L; Hamstra, M; Harvey, P J; Hearns, C; Jillings, C J; Kamaev, O; Kemp, A; Kuzniak, M; Langrock, S; La Zia, F.
Afiliación
  • Amaudruz PA; TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
  • Baldwin M; Rutherford Appleton Laboratory, Harwell Oxford, Didcot OX11 0QX, United Kingdom.
  • Batygov M; Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario P3E 2C6, Canada.
  • Beltran B; Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada.
  • Bina CE; Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada.
  • Bishop D; TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
  • Bonatt J; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Boorman G; Royal Holloway University London, Egham Hill, Egham, Surrey TW20 0EX, United Kingdom.
  • Boulay MG; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Broerman B; Department of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada.
  • Bromwich T; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Bueno JF; University of Sussex, Sussex House, Brighton, East Sussex BN1 9RH, United Kingdom.
  • Burghardt PM; Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada.
  • Butcher A; Department of Physics, Technische Universität München, 80333 Munich, Germany.
  • Cai B; Royal Holloway University London, Egham Hill, Egham, Surrey TW20 0EX, United Kingdom.
  • Chan S; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Chen M; TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
  • Chouinard R; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Cleveland BT; Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada.
  • Cranshaw D; Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario P3E 2C6, Canada.
  • Dering K; SNOLAB, Lively, Ontario P3Y 1M3, Canada.
  • DiGioseffo J; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Dittmeier S; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Duncan FA; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Dunford M; TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
  • Erlandson A; Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario P3E 2C6, Canada.
  • Fatemighomi N; SNOLAB, Lively, Ontario P3Y 1M3, Canada.
  • Florian S; Department of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada.
  • Flower A; Department of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada.
  • Ford RJ; Canadian Nuclear Laboratories Ltd, Chalk River, Ontario K0J 1J0, Canada.
  • Gagnon R; Royal Holloway University London, Egham Hill, Egham, Surrey TW20 0EX, United Kingdom.
  • Giampa P; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Golovko VV; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Gorel P; Department of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada.
  • Gornea R; Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario P3E 2C6, Canada.
  • Grace E; SNOLAB, Lively, Ontario P3Y 1M3, Canada.
  • Graham K; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Gulyev E; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Hakobyan R; Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario K7L 3N6, Canada.
  • Hall A; Canadian Nuclear Laboratories Ltd, Chalk River, Ontario K0J 1J0, Canada.
  • Hallin AL; Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario P3E 2C6, Canada.
  • Hamstra M; Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada.
  • Harvey PJ; SNOLAB, Lively, Ontario P3Y 1M3, Canada.
  • Hearns C; Department of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada.
  • Jillings CJ; Royal Holloway University London, Egham Hill, Egham, Surrey TW20 0EX, United Kingdom.
  • Kamaev O; Department of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada.
  • Kemp A; TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
  • Kuzniak M; Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada.
  • Langrock S; Royal Holloway University London, Egham Hill, Egham, Surrey TW20 0EX, United Kingdom.
  • La Zia F; Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada.
Phys Rev Lett ; 121(7): 071801, 2018 Aug 17.
Article en En | MEDLINE | ID: mdl-30169081
This Letter reports the first results of a direct dark matter search with the DEAP-3600 single-phase liquid argon (LAr) detector. The experiment was performed 2 km underground at SNOLAB (Sudbury, Canada) utilizing a large target mass, with the LAr target contained in a spherical acrylic vessel of 3600 kg capacity. The LAr is viewed by an array of PMTs, which would register scintillation light produced by rare nuclear recoil signals induced by dark matter particle scattering. An analysis of 4.44 live days (fiducial exposure of 9.87 ton day) of data taken during the initial filling phase demonstrates the best electronic recoil rejection using pulse-shape discrimination in argon, with leakage <1.2×10^{-7} (90% C.L.) between 15 and 31 keV_{ee}. No candidate signal events are observed, which results in the leading limit on weakly interacting massive particle (WIMP)-nucleon spin-independent cross section on argon, <1.2×10^{-44} cm^{2} for a 100 GeV/c^{2} WIMP mass (90% C.L.).

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2018 Tipo del documento: Article País de afiliación: Canadá

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2018 Tipo del documento: Article País de afiliación: Canadá