First Direct Detection Constraints on Planck-Scale Mass Dark Matter with Multiple-Scatter Signatures Using the DEAP-3600 Detector
Affiliations
- 1 Department of Physics, Carleton University, Ottawa, Ontario, K1S 5B6, Canada.
- 2 Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Queen's University, Kingston ON K7L 3N6,Canada.
- 3 Instituto de Física, Universidad Nacional Autónoma de México, A.P. 20-364, México D.F. 01000, México.
- 4 Department of Physics, University of Alberta, Edmonton, Alberta, T6G 2R3, Canada.
- 5 Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario, K7L 3N6, Canada.
- 6 INFN Cagliari, Cagliari 09042, Italy.
- 7 Physics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy.
- 8 Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain.
- 9 Physics Department, Università degli Studi "Federico II" di Napoli, Napoli 80126, Italy.
- 10 Astronomical Observatory of Capodimonte, Salita Moiariello 16, I-80131 Napoli, Italy.
- 11 INFN Napoli, Napoli 80126, Italy.
- 12 Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario, P3E 2C6, Canada.
- 13 SNOLAB, Lively, Ontario, P3Y 1N2, Canada.
- 14 PRISMA+, Cluster of Excellence and Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, 55128 Mainz, Germany.
- 15 Canadian Nuclear Laboratories, Chalk River, Ontario, K0J 1J0, Canada.
- 16 Royal Holloway University London, Egham Hill, Egham, Surrey TW20 0EX, United Kingdom.
- 17 TRIUMF, Vancouver, British Columbia, V6T 2A3, Canada.
- 18 National Research Centre Kurchatov Institute, Moscow 123182, Russia.
- 19 National Research Nuclear University MEPhI, Moscow 115409, Russia.
- 20 AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Rektorska 4, 00-614 Warsaw, Poland.
- 21 INFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy.
- 22 Department of Physics, Technische Universität München, 80333 Munich, Germany.
- 23 Physics Department, Princeton University, Princeton, New Jersey 08544, USA.
- 24 University of Sussex, Sussex House, Brighton, East Sussex BN1 9RH, United Kingdom.
- 25 BP2, National Centre for Nuclear Research, ul. Pasteura 7, 02-093 Warsaw, Poland.
- PMID: 35061499
- DOI: 10.1103/PhysRevLett.128.011801
First Direct Detection Constraints on Planck-Scale Mass Dark Matter with Multiple-Scatter Signatures Using the DEAP-3600 Detector
Authors
Affiliations
- 1 Department of Physics, Carleton University, Ottawa, Ontario, K1S 5B6, Canada.
- 2 Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Queen's University, Kingston ON K7L 3N6,Canada.
- 3 Instituto de Física, Universidad Nacional Autónoma de México, A.P. 20-364, México D.F. 01000, México.
- 4 Department of Physics, University of Alberta, Edmonton, Alberta, T6G 2R3, Canada.
- 5 Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario, K7L 3N6, Canada.
- 6 INFN Cagliari, Cagliari 09042, Italy.
- 7 Physics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy.
- 8 Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain.
- 9 Physics Department, Università degli Studi "Federico II" di Napoli, Napoli 80126, Italy.
- 10 Astronomical Observatory of Capodimonte, Salita Moiariello 16, I-80131 Napoli, Italy.
- 11 INFN Napoli, Napoli 80126, Italy.
- 12 Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario, P3E 2C6, Canada.
- 13 SNOLAB, Lively, Ontario, P3Y 1N2, Canada.
- 14 PRISMA+, Cluster of Excellence and Institut für Kernphysik, Johannes Gutenberg-Universität Mainz, 55128 Mainz, Germany.
- 15 Canadian Nuclear Laboratories, Chalk River, Ontario, K0J 1J0, Canada.
- 16 Royal Holloway University London, Egham Hill, Egham, Surrey TW20 0EX, United Kingdom.
- 17 TRIUMF, Vancouver, British Columbia, V6T 2A3, Canada.
- 18 National Research Centre Kurchatov Institute, Moscow 123182, Russia.
- 19 National Research Nuclear University MEPhI, Moscow 115409, Russia.
- 20 AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Rektorska 4, 00-614 Warsaw, Poland.
- 21 INFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy.
- 22 Department of Physics, Technische Universität München, 80333 Munich, Germany.
- 23 Physics Department, Princeton University, Princeton, New Jersey 08544, USA.
- 24 University of Sussex, Sussex House, Brighton, East Sussex BN1 9RH, United Kingdom.
- 25 BP2, National Centre for Nuclear Research, ul. Pasteura 7, 02-093 Warsaw, Poland.
- PMID: 35061499
- DOI: 10.1103/PhysRevLett.128.011801
Abstract
Dark matter with Planck-scale mass (≃10^{19} GeV/c^{2}) arises in well-motivated theories and could be produced by several cosmological mechanisms. A search for multiscatter signals from supermassive dark matter was performed with a blind analysis of data collected over a 813 d live time with DEAP-3600, a 3.3 t single-phase liquid argon-based detector at SNOLAB. No candidate signals were observed, leading to the first direct detection constraints on Planck-scale mass dark matter. Leading limits constrain dark matter masses between 8.3×10^{6} and 1.2×10^{19} GeV/c^{2}, and ^{40}Ar-scattering cross sections between 1.0×10^{-23} and 2.4×10^{-18} cm^{2}. These results are interpreted as constraints on composite dark matter models with two different nucleon-to-nuclear cross section scalings.
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