Relative measurement and extrapolation of the scintillation quenching factor of $$\alpha $$-particles in liquid argon using DEAP-3600 data

Abstract The knowledge of scintillation quenching of $$\alpha $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>α</mml:mi> </mml:math> -particles plays a paramount role in understanding $$\alpha $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>α</mml:mi> </mml:math> -induced backgrounds and improving the sensitivity of liquid argon-based direct detection of dark matter experiments. We performed a relative measurement of scintillation quenching in the MeV energy region using radioactive isotopes ( $$^{222}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>222</mml:mn> </mml:mmultiscripts> </mml:math> Rn, $$^{218}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>218</mml:mn> </mml:mmultiscripts> </mml:math> Po and $$^{214}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>214</mml:mn> </mml:mmultiscripts> </mml:math> Po isotopes) present in trace amounts in the DEAP-3600 detector and quantified the uncertainty of extrapolating the quenching factor to the low-energy region.

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Publication Details

Journal
The European Physical Journal C
Published
2025-01-27
DOI
https://doi.org/10.1140/epjc/s10052-024-13518-7
Citations
1
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
1.87

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article

Relative measurement and extrapolation of the scintillation quenching factor of $$\alpha $$-particles in liquid argon using DEAP-3600 data

A. B. McDonald, C. Rethmeier, D. Gahan, N. Levashko et al.
1 citations
The European Physical Journal C
Dark Matter and Cosmic Phenomena
1.87
article

Relative measurement and extrapolation of the scintillation quenching factor of $$\alpha $$-particles in liquid argon using DEAP-3600 data

A. B. McDonald, C. Rethmeier, D. Gahan, N. Levashko, S. Viel, J. Monroe, M. Laí, A. Erlandson, Leszek Roszkowski, E. Ellingwood, M. Lissia, K. Graham, Beomjun Park, V. Pesudo, A. Moharana, M. G. Boulay, F. Retière, M. Cárdenas-Montes, Apexa Maru, F. Rad, K. Sobotkiewich, M. Dunford, G. Kaur, James Mason, B. Cai, L. Doria, W. Bonivento, J. Sosiak, M. Alpízar-Venegas, A. Murray, C. Mielnichuk, J. Hucker, M. Hamstra, L. Luzzi, Mehran Yazdi, D. J. Auty, J. Walding, M. G. Perry, V. Shalamova, R. Santorelli, J. Soukup, P. Amaudruz, B. Jigmeddorj, P. García Abia, T. Sonley, B. Vyas, E. Vázquez-Jáuregui, C. E. Bina, D. Goeldi, B. Beltran, D. Papi, C. Ng, P. Skensved, T. McElroy, S. Choudhary, P. DelGobbo, T. Smirnova, A. Giménez-Alcázar, S. Seth, P. Giampa, R. Crampton, G. Dolganov, A. Ilyasov, Sanjoy Kumar Pal, M. Walczak, S. Haskins, M. Kuźniak, T. R. Pollmann, D. Gallacher, P. Gorel, P. C. F. Di Stefano, R. Stainforth, A. L. Hallin, James Anstey, S. S. Farahani, B. Lehnert, T. Hugues, G. Oliviéro, L. Mirasola, G. Fiorillo, M. Stringer, J. Tang, S. Westerdale, A. Kemp, S. Garg, Jia Hu, Michał Olszewski, N. Fatemighomi, I. Machulin, F. La Zia, M. Ward, S. J. Daugherty, B. T. Cleveland, F. A. Duncan, C. Jillings, J. F. Bueno, M. Batygov, S. Langrock, R. Ford, F. G. Schuckman, P. Adhikari, J. B. McLaughlin, R. Wormington
article en
1 citations

Abstract

Abstract The knowledge of scintillation quenching of $$\alpha $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>α</mml:mi> </mml:math> -particles plays a paramount role in understanding $$\alpha $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>α</mml:mi> </mml:math> -induced backgrounds and improving the sensitivity of liquid argon-based direct detection of dark matter experiments. We performed a relative measurement of scintillation quenching in the MeV energy region using radioactive isotopes ( $$^{222}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>222</mml:mn> </mml:mmultiscripts> </mml:math> Rn, $$^{218}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>218</mml:mn> </mml:mmultiscripts> </mml:math> Po and $$^{214}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>214</mml:mn> </mml:mmultiscripts> </mml:math> Po isotopes) present in trace amounts in the DEAP-3600 detector and quantified the uncertainty of extrapolating the quenching factor to the low-energy region.

The European Physical Journal CVol. 85(1)
Lawrence Berkeley National Laboratory (US), University of Alberta (CA), University of Cagliari (IT), Royal Holloway University of London (GB), Johannes Gutenberg University Mainz (DE), Queen's University (CA), Kurchatov Institute (RU), University of California System (US), National Institute for Subatomic Physics (NL), Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (IT), National Centre for Social research (GR), Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES), Canadian Nuclear Laboratories (CA), Laurentian University (CA), Technical University of Munich (DE), Carleton University (CA), University of Naples Federico II (IT), National Research Nuclear University MEPhI (RU), Universidad Nacional Autónoma de México (MX), Polish Academy of Sciences (PL)
Fundación Marcos Moshinsky, Comunidad de Madrid, Ministry of Advanced Education, Government of Alberta, University of Alberta, Leverhulme Trust, Fundacja na rzecz Nauki Polskiej, Consejo Nacional de Ciencia y Tecnología, Queen's University, Ministerio de Ciencia e Innovación, Russian Science Foundation, Canada First Research Excellence Fund, Alliance de recherche numérique du Canada, South East Physics Network, Natural Sciences and Engineering Research Council of Canada, Science and Technology Facilities Council, Leibniz-Gemeinschaft, Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México, European Regional Development Fund, Ontario Ministry of Research and Innovation
Openalex Percentile: Top 16%
Dark Matter and Cosmic Phenomena
1.87
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