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arXiv · 2608.20504

Measurement of the muon flux at SNOLAB using the DEAP-3600 experiment

DEAP Collaboration·P. Adhikari·M. Alpízar-Venegas·P. -A. Amaudruz·D. J. Auty·M. Batygov·B. Beltran·M. A. Bigentini·C. E. Bina·W. Bonivento·M. G. Boulay·J. F. Bueno·M. Cadeddu·B. Cai·M. Cárdenas-Montes·N. Cargioli·S. Cavuoti·S. Choudhary·B. T. Cleveland·R. Crampton·E. Darling·S. Daugherty·P. Di Stefano·G. Dolganov·L. Doria·F. A. Duncan·M. Dunford·E. Ellingwood·A. Erlandson·S. S. Farahani·N. Fatemighomi·L. Ferro·G. Fiorillo·R. J. Ford·A. Garai·P. García Abia·S. Garg·P. Giampa·A. Giménez-Alcázar·D. Goeldi·P. Gorel·K. Graham·A. L. Hallin·M. Hamstra·S. Haskins·J. Hu·J. Hucker·D. Huff·T. Hugues·A. Ilyasov·B. Jigmeddorj·C. J. Jillings·G. Kaur·A. Kemp·M. Khoshraftar Yazdi·G. Killaire·M. Kuźniak·F. La Zia·M. Lai·S. Langrock·B. Lehnert·M. Lissia·L. Luzzi·I. Machulin·S. MacKenzie·A. Maru·J. Mason·A. B. McDonald·T. McElroy·J. B. McLaughlin·C. Mielnichuk·L. Mirasola·S. Mohanty·A. Moharana·J. Monroe·A. Murray·M. Needs·C. Ng·G. Nieradka·G. Oliviéro·M. Olszewski·S. Pal·D. Papi·B. Park·R. Pavarani·M. Perry·V. Pesudo·T. R. Pollmann·F. Rad·C. Rethmeier·F. Retière·L. Roszkowski·R. Santorelli·F. G. Schuckman II·M. Sestu·S. Seth·V. Shalamova·P. Skensved·T. Smirnova·K. Sobotkiewich
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Abstract

A direct measurement of the muon flux at SNOLAB is performed using the DEAP-3600 experiment, located 2 km underground at SNOLAB near Sudbury, Canada. Primarily designed for the direct detection of weakly interacting massive particles (WIMPs), a dark matter candidate, DEAP-3600 consists of an inner spherical acrylic vessel containing a liquid argon target; this vessel is enclosed within a steel shell which is submerged in an instrumented water tank, serving as a muon veto for the dark matter search. The muon flux measurement is performed using a cut-and-count analysis of events observed in the muon veto detector and of events which are coincident between the muon veto and the liquid argon target. The requirement that muons traverse both the water and liquid argon minimizes instrumental backgrounds and systematic uncertainties. Using data collected from November 2016 to March 2020, the muon flux is measured by this coincidence analysis to be $(3.71 \pm 0.25_{\textrm{stat}} \pm 0.09_{\textrm{sys}}) \times 10^{-10}\, \mu/$cm$^2$/s. The standalone measurement using muon veto data only is compatible within uncertainties. Both measurements agree with the previous result by the SNO experiment and with simulations carried out using the MUTE software. These results provide an important benchmark for future rare-event searches at the SNOLAB facility.

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DEAP Collaboration, P. Adhikari, M. Alpízar-Venegas, P. -A. Amaudruz, D. J. Auty, M. Batygov, B. Beltran, M. A. Bigentini, C. E. Bina, W. Bonivento, M. G. Boulay, J. F. Bueno, M. Cadeddu, B. Cai, M. Cárdenas-Montes, N. Cargioli, S. Cavuoti, S. Choudhary, B. T. Cleveland, R. Crampton, E. Darling, S. Daugherty, P. Di Stefano, G. Dolganov, L. Doria, F. A. Duncan, M. Dunford, E. Ellingwood, A. Erlandson, S. S. Farahani, N. Fatemighomi, L. Ferro, G. Fiorillo, R. J. Ford, A. Garai, P. García Abia, S. Garg, P. Giampa, A. Giménez-Alcázar, D. Goeldi, P. Gorel, K. Graham, A. L. Hallin, M. Hamstra, S. Haskins, J. Hu, J. Hucker, D. Huff, T. Hugues, A. Ilyasov, B. Jigmeddorj, C. J. Jillings, G. Kaur, A. Kemp, M. Khoshraftar Yazdi, G. Killaire, M. Kuźniak, F. La Zia, M. Lai, S. Langrock, B. Lehnert, M. Lissia, L. Luzzi, I. Machulin, S. MacKenzie, A. Maru, J. Mason, A. B. McDonald, T. McElroy, J. B. McLaughlin, C. Mielnichuk, L. Mirasola, S. Mohanty, A. Moharana, J. Monroe, A. Murray, M. Needs, C. Ng, G. Nieradka, G. Oliviéro, M. Olszewski, S. Pal, D. Papi, B. Park, R. Pavarani, M. Perry, V. Pesudo, T. R. Pollmann, F. Rad, C. Rethmeier, F. Retière, L. Roszkowski, R. Santorelli, F. G. Schuckman II, M. Sestu, S. Seth, V. Shalamova, P. Skensved, T. Smirnova, K. Sobotkiewich. 2026-08-20. Measurement of the muon flux at SNOLAB using the DEAP-3600 experiment. https://arxiv.org/abs/2608.20504

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