Muon-induced background in a next-generation dark matter experiment based on liquid xenon
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Published version
Author(s)
Pec, Viktor
Kudryavtsev, Vitaly A
Araujo, Henrique M
Sumner, Timothy J
Type
Journal Article
Abstract
Muon-induced neutrons can lead to potentially irreducible backgrounds in rare event search experiments. We have investigated the implication of laboratory depth on the muon-induced background in a future dark matter experiment capable of reaching the so-called neutrino floor. Our simulation study focused on a xenon-based detector with 70 tonnes of active mass, surrounded by additional veto systems plus a water shield. Two locations at the Boulby Underground Laboratory (UK) were analysed as examples: an experimental cavern in salt at a depth of 2850 m w. e. (similar to the location of the existing laboratory), and a deeper laboratory located in polyhalite rock at a depth of 3575 m w. e. Our results show that no cosmogenic background events are likely to survive standard analysis cuts for 10 years of operation at either location. The largest background component we identified comes from beta-delayed neutron emission from
Date Issued
2024-05
Date Acceptance
2024-04-08
Citation
European Physical Journal C: Particles and Fields, 2024, 84 (5)
ISSN
1124-1861
Publisher
SpringerOpen
Journal / Book Title
European Physical Journal C: Particles and Fields
Volume
84
Issue
5
Copyright Statement
© The Author(s) 2024
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
License URL
Identifier
https://link.springer.com/article/10.1140/epjc/s10052-024-12768-9
Subjects
COSMIC-RAY MUONS
FLUX
INDUCED NEUTRON YIELD
Physical Sciences
Physics
Physics, Particles & Fields
PROPAGATION
Science & Technology
SCINTILLATOR
SIMULATION
Publication Status
Published
Article Number
481
Date Publish Online
2024-05-09