Dark matter with Planck-scale mass (?1019 GeV/c2) 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 8.3×106 and 1.2×1019 GeV/c2, and Ar40-scattering cross sections between 1.0×10-23 and 2.4×10-18 cm2. These results are interpreted as constraints on composite dark matter models with two different nucleon-to-nuclear cross section scalings.

First Direct Detection Constraints on Planck-Scale Mass Dark Matter with Multiple-Scatter Signatures Using the DEAP-3600 Detector / Adhikari, P.; Ajaj, R.; Alpizar-Venegas, M.; Auty, D.; Benmansour, H.; Bina, C.; Bonivento, W.; Boulay, M.; Cadeddu, M.; Cai, B.; Cardenas-Montes, M.; Cavuoti, S.; Chen, Y.; Cleveland, B.; Corning, J.; Daugherty, S.; Delgobbo, P.; Di Stefano, P.; Doria, L.; Dunford, M.; Ellingwood, E.; Erlandson, A.; Farahani, S.; Fatemighomi, N.; Fiorillo, G.; Gallacher, D.; Garcia Abia, P.; Garg, S.; Giampa, P.; Goeldi, D.; Gorel, P.; Graham, K.; Grobov, A.; Hallin, A.; Hamstra, M.; Hugues, T.; Ilyasov, A.; Joy, A.; Jigmeddorj, B.; Jillings, C.; Kamaev, O.; Kaur, G.; Kemp, A.; Kochanek, I.; Kuzniak, M.; Lai, M.; Langrock, S.; Lehnert, B.; Leonhardt, A.; Levashko, N.; Li, X.; Lissia, M.; Litvinov, O.; Lock, J.; Longo, G.; Machulin, I.; Mcdonald, A. B.; Mcelroy, T.; Mclaughlin, J.; Mielnichuk, C.; Mirasola, L.; Monroe, J.; Oliviero, G.; Pal, S.; Peeters, S.; Perry, M.; Pesudo, V.; Picciau, E.; Piro, M. -C.; Pollmann, T. R.; Raj, N.; Rand, E.; Rethmeier, C.; Retiere, F.; Rodriguez-Garcia, I.; Roszkowski, L.; Ruhland, J. B.; Sanchez Garcia, E.; Sanchez-Pastor, T.; Santorelli, R.; Seth, S.; Sinclair, D.; Skensved, P.; Smith, B.; Smith, N. J. T.; Sonley, T.; Stainforth, R.; Stringer, M.; Sur, B.; Vazquez-Jauregui, E.; Viel, S.; Walding, J.; Waqar, M.; Ward, M.; Westerdale, S.; Willis, J.; Zuniga-Reyes, A.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 128:1(2022), p. 011801. [10.1103/PhysRevLett.128.011801]

First Direct Detection Constraints on Planck-Scale Mass Dark Matter with Multiple-Scatter Signatures Using the DEAP-3600 Detector

Cavuoti S.;Fiorillo G.;Longo G.;
2022

Abstract

Dark matter with Planck-scale mass (?1019 GeV/c2) 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 8.3×106 and 1.2×1019 GeV/c2, and Ar40-scattering cross sections between 1.0×10-23 and 2.4×10-18 cm2. These results are interpreted as constraints on composite dark matter models with two different nucleon-to-nuclear cross section scalings.
2022
First Direct Detection Constraints on Planck-Scale Mass Dark Matter with Multiple-Scatter Signatures Using the DEAP-3600 Detector / Adhikari, P.; Ajaj, R.; Alpizar-Venegas, M.; Auty, D.; Benmansour, H.; Bina, C.; Bonivento, W.; Boulay, M.; Cadeddu, M.; Cai, B.; Cardenas-Montes, M.; Cavuoti, S.; Chen, Y.; Cleveland, B.; Corning, J.; Daugherty, S.; Delgobbo, P.; Di Stefano, P.; Doria, L.; Dunford, M.; Ellingwood, E.; Erlandson, A.; Farahani, S.; Fatemighomi, N.; Fiorillo, G.; Gallacher, D.; Garcia Abia, P.; Garg, S.; Giampa, P.; Goeldi, D.; Gorel, P.; Graham, K.; Grobov, A.; Hallin, A.; Hamstra, M.; Hugues, T.; Ilyasov, A.; Joy, A.; Jigmeddorj, B.; Jillings, C.; Kamaev, O.; Kaur, G.; Kemp, A.; Kochanek, I.; Kuzniak, M.; Lai, M.; Langrock, S.; Lehnert, B.; Leonhardt, A.; Levashko, N.; Li, X.; Lissia, M.; Litvinov, O.; Lock, J.; Longo, G.; Machulin, I.; Mcdonald, A. B.; Mcelroy, T.; Mclaughlin, J.; Mielnichuk, C.; Mirasola, L.; Monroe, J.; Oliviero, G.; Pal, S.; Peeters, S.; Perry, M.; Pesudo, V.; Picciau, E.; Piro, M. -C.; Pollmann, T. R.; Raj, N.; Rand, E.; Rethmeier, C.; Retiere, F.; Rodriguez-Garcia, I.; Roszkowski, L.; Ruhland, J. B.; Sanchez Garcia, E.; Sanchez-Pastor, T.; Santorelli, R.; Seth, S.; Sinclair, D.; Skensved, P.; Smith, B.; Smith, N. J. T.; Sonley, T.; Stainforth, R.; Stringer, M.; Sur, B.; Vazquez-Jauregui, E.; Viel, S.; Walding, J.; Waqar, M.; Ward, M.; Westerdale, S.; Willis, J.; Zuniga-Reyes, A.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 128:1(2022), p. 011801. [10.1103/PhysRevLett.128.011801]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/878873
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