European Physical Journal C: Particles and Fields (Jul 2025)
Direct measurement of the $$^{39}$$ 39 Ar half-life from 3.4 years of data with the DEAP-3600 detector
- P. Adhikari,
- R. Ajaj,
- M. Alpízar-Venegas,
- P.-A. Amaudruz,
- J. Anstey,
- D. J. Auty,
- M. Batygov,
- B. Beltran,
- M. A. Bigentini,
- C. E. Bina,
- W. M. Bonivento,
- M. G. Boulay,
- J. F. Bueno,
- M. Cadeddu,
- B. Cai,
- M. Cárdenas-Montes,
- S. Cavuoti,
- Y. Chen,
- S. Choudhary,
- B. T. Cleveland,
- R. Crampton,
- S. Daugherty,
- P. DelGobbo,
- P. Di Stefano,
- G. Dolganov,
- L. Doria,
- F. A. Duncan,
- M. Dunford,
- E. Ellingwood,
- A. Erlandson,
- S. S. Farahani,
- N. Fatemighomi,
- G. Fiorillo,
- R. J. Ford,
- D. Gahan,
- D. Gallacher,
- A. Garai,
- P. García Abia,
- S. Garg,
- P. Giampa,
- A. Giménez-Alcázar,
- D. Goeldi,
- V. V. Golovko,
- P. Gorel,
- K. Graham,
- A. Grobov,
- A. L. Hallin,
- M. Hamstra,
- S. Haskins,
- J. Hu,
- J. Hucker,
- T. Hugues,
- A. Ilyasov,
- B. Jigmeddorj,
- C. J. Jillings,
- A. Joy,
- G. Kaur,
- A. Kemp,
- M. Khoshraftar Yazdi,
- M. Kuźniak,
- F. La Zia,
- M. Lai,
- S. Langrock,
- B. Lehnert,
- J. LePage-Bourbonnais,
- N. Levashko,
- M. Lissia,
- L. Luzzi,
- I. Machulin,
- A. Maru,
- J. Mason,
- A. B. McDonald,
- T. McElroy,
- J. B. McLaughlin,
- C. Mielnichuk,
- L. Mirasola,
- A. Moharana,
- J. Monroe,
- A. Murray,
- C. Ng,
- G. Oliviéro,
- M. Olszewski,
- S. Pal,
- D. Papi,
- B. Park,
- M. Perry,
- V. Pesudo,
- T. R. Pollmann,
- F. Rad,
- C. Rethmeier,
- F. Retière,
- I. Rodríguez García,
- L. Roszkowski,
- R. Santorelli,
- F. G. Schuckman II,
- S. Seth,
- V. Shalamova,
- P. Skensved,
- T. Smirnova,
- K. Sobotkiewich,
- T. Sonley,
- J. Sosiak,
- J. Soukup,
- R. Stainforth,
- M. Stringer,
- J. Tang,
- R. Turcotte-Tardif,
- E. Vázquez-Jáuregui,
- S. Viel,
- B. Vyas,
- M. Walczak,
- J. Walding,
- M. Ward,
- S. Westerdale,
- R. Wormington,
- A. Zuñiga-Reyes,
- DEAP Collaboration
Affiliations
- P. Adhikari
- Department of Physics, Carleton University
- R. Ajaj
- Department of Physics, Carleton University
- M. Alpízar-Venegas
- Instituto de Física, Universidad Nacional Autónoma de México
- P.-A. Amaudruz
- TRIUMF
- J. Anstey
- Department of Physics, Carleton University
- D. J. Auty
- Department of Physics, University of Alberta
- M. Batygov
- School of Natural Sciences, Laurentian University
- B. Beltran
- Department of Physics, University of Alberta
- M. A. Bigentini
- Department of Physics, Carleton University
- C. E. Bina
- Department of Physics, University of Alberta
- W. M. Bonivento
- INFN Cagliari
- M. G. Boulay
- Department of Physics, Carleton University
- J. F. Bueno
- Department of Physics, University of Alberta
- M. Cadeddu
- INFN Cagliari
- B. Cai
- Department of Physics, Carleton University
- M. Cárdenas-Montes
- Centro de Investigaciones Energénticas, Medioambientales y Tecnológicas
- S. Cavuoti
- INFN Napoli
- Y. Chen
- Department of Physics, University of Alberta
- S. Choudhary
- AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences
- B. T. Cleveland
- School of Natural Sciences, Laurentian University
- R. Crampton
- Department of Physics, Carleton University
- S. Daugherty
- Department of Physics, Carleton University
- P. DelGobbo
- Department of Physics, Carleton University
- P. Di Stefano
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- G. Dolganov
- National Research Centre Kurchatov Institute
- L. Doria
- PRISMA+ Cluster of Excellence, Institut für Kernphysik, Johannes Gutenberg-Universität Mainz
- F. A. Duncan
- Department of Physics, University of Alberta
- M. Dunford
- Department of Physics, Carleton University
- E. Ellingwood
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- A. Erlandson
- Canadian Nuclear Laboratories
- S. S. Farahani
- Department of Physics, University of Alberta
- N. Fatemighomi
- Royal Holloway University London
- G. Fiorillo
- Physics Department, Università degli Studi “Federico II” di Napoli
- R. J. Ford
- School of Natural Sciences, Laurentian University
- D. Gahan
- Physics Department, Università degli Studi di Cagliari
- D. Gallacher
- Department of Physics, Carleton University
- A. Garai
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- P. García Abia
- Centro de Investigaciones Energénticas, Medioambientales y Tecnológicas
- S. Garg
- Department of Physics, Carleton University
- P. Giampa
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- A. Giménez-Alcázar
- Centro de Investigaciones Energénticas, Medioambientales y Tecnológicas
- D. Goeldi
- Department of Physics, Carleton University
- V. V. Golovko
- Canadian Nuclear Laboratories
- P. Gorel
- School of Natural Sciences, Laurentian University
- K. Graham
- Department of Physics, Carleton University
- A. Grobov
- National Research Centre Kurchatov Institute
- A. L. Hallin
- Department of Physics, University of Alberta
- M. Hamstra
- Department of Physics, Carleton University
- S. Haskins
- Department of Physics, Carleton University
- J. Hu
- Department of Physics, University of Alberta
- J. Hucker
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- T. Hugues
- AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences
- A. Ilyasov
- National Research Centre Kurchatov Institute
- B. Jigmeddorj
- School of Natural Sciences, Laurentian University
- C. J. Jillings
- School of Natural Sciences, Laurentian University
- A. Joy
- Department of Physics, University of Alberta
- G. Kaur
- Department of Physics, Carleton University
- A. Kemp
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- M. Khoshraftar Yazdi
- Department of Physics, University of Alberta
- M. Kuźniak
- AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences
- F. La Zia
- Royal Holloway University London
- M. Lai
- Physics Department, Università degli Studi di Cagliari
- S. Langrock
- School of Natural Sciences, Laurentian University
- B. Lehnert
- Nuclear Science Division, Lawrence Berkeley National Laboratory
- J. LePage-Bourbonnais
- Department of Physics, Carleton University
- N. Levashko
- National Research Centre Kurchatov Institute
- M. Lissia
- INFN Cagliari
- L. Luzzi
- Centro de Investigaciones Energénticas, Medioambientales y Tecnológicas
- I. Machulin
- National Research Centre Kurchatov Institute
- A. Maru
- Department of Physics, Carleton University
- J. Mason
- Department of Physics, Carleton University
- A. B. McDonald
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- T. McElroy
- Department of Physics, University of Alberta
- J. B. McLaughlin
- Royal Holloway University London
- C. Mielnichuk
- Department of Physics, University of Alberta
- L. Mirasola
- Physics Department, Università degli Studi di Cagliari
- A. Moharana
- Department of Physics, Carleton University
- J. Monroe
- Royal Holloway University London
- A. Murray
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- C. Ng
- Department of Physics, University of Alberta
- G. Oliviéro
- Department of Physics, Carleton University
- M. Olszewski
- AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences
- S. Pal
- Department of Physics, University of Alberta
- D. Papi
- Department of Physics, University of Alberta
- B. Park
- Department of Physics, University of Alberta
- M. Perry
- Department of Physics, Carleton University
- V. Pesudo
- Centro de Investigaciones Energénticas, Medioambientales y Tecnológicas
- T. R. Pollmann
- School of Natural Sciences, Laurentian University
- F. Rad
- Department of Physics, Carleton University
- C. Rethmeier
- Department of Physics, Carleton University
- F. Retière
- TRIUMF
- I. Rodríguez García
- Centro de Investigaciones Energénticas, Medioambientales y Tecnológicas
- L. Roszkowski
- AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences
- R. Santorelli
- Centro de Investigaciones Energénticas, Medioambientales y Tecnológicas
- F. G. Schuckman II
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- S. Seth
- Department of Physics, Carleton University
- V. Shalamova
- Department of Physics and Astronomy, University of California
- P. Skensved
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- T. Smirnova
- Department of Physics and Astronomy, University of California
- K. Sobotkiewich
- Department of Physics, Carleton University
- T. Sonley
- Department of Physics, Carleton University
- J. Sosiak
- Department of Physics, Carleton University
- J. Soukup
- Department of Physics, University of Alberta
- R. Stainforth
- Department of Physics, Carleton University
- M. Stringer
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- J. Tang
- Department of Physics, University of Alberta
- R. Turcotte-Tardif
- Department of Physics, Carleton University
- E. Vázquez-Jáuregui
- Instituto de Física, Universidad Nacional Autónoma de México
- S. Viel
- Department of Physics, Carleton University
- B. Vyas
- Department of Physics, Carleton University
- M. Walczak
- AstroCeNT, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences
- J. Walding
- Royal Holloway University London
- M. Ward
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- S. Westerdale
- Department of Physics and Astronomy, University of California
- R. Wormington
- Department of Physics, Engineering Physics and Astronomy, Queen’s University
- A. Zuñiga-Reyes
- Instituto de Física, Universidad Nacional Autónoma de México
- DEAP Collaboration
- Department of Physics, Carleton University
- DOI
- https://doi.org/10.1140/epjc/s10052-025-14289-5
- Journal volume & issue
-
Vol. 85,
no. 7
pp. 1 – 11
Abstract
Abstract The half-life of $$^{39}$$ 39 Ar is measured using the DEAP-3600 detector located 2 km underground at SNOLAB. Between 2016 and 2020, DEAP-3600 used a target mass of (3269 ± 24) kg of liquid argon distilled from the atmosphere in a direct-detection dark matter search. Such an argon mass also enables direct measurements of argon isotope properties. The decay of $$^{39}$$ 39 Ar in DEAP-3600 is the dominant source of triggers by two orders of magnitude, ensuring high statistics and making DEAP-3600 well-suited for measuring this isotope’s half-life. Use of the pulse-shape discrimination technique in DEAP-3600 allows powerful discrimination between nuclear recoils and electron recoils, resulting in the selection of a clean sample of $$^{39}$$ 39 Ar decays. Observing over a period of 3.4 years, the $$^{39}$$ 39 Ar half-life is measured to be $$(302 \pm 8_\textrm{stat} \pm 6_\textrm{sys})$$ ( 302 ± 8 stat ± 6 sys ) years. This new direct measurement suggests that the half-life of $$^{39}$$ 39 Ar is significantly longer than the accepted value, with potential implications for measurements using this isotope’s half-life as input.