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Study of Cosmogenic Activation above Ground for the DarkSide-20k Experiment

Astroparticle Physics(2023)SCI 3区

Univ Calif Davis | Gran Sasso Sci Inst | Polish Acad Sci | INFN Catania | Univ Sao Paulo | Pacific Northwest Natl Lab | Augustana Univ | TRIUMF | INFN Cagliari | Instituto de Física | Mendeleev Univ Chem Technol | INFN Lab Nazl Legnaro | Royal Holloway Univ London | Aix Marseille Univ | INFN Napoli | INFN Pisa | INFN Sez Roma | Univ Genoa | Carleton Univ | INFN Genova | INFN Lab Nazl Gran Sasso | Univ Zaragoza | CIEMAT | Lomonosov Moscow State Univ | Univ Bologna | INFN Milano | SNOLAB | Jagiellonian Univ | INFN Torino | Univ Salerno | St Petersburg Nucl Phys Inst | Queens Univ | Kurchatov Inst | Univ Paris | Princeton Univ | Swiss Fed Inst Technol | Univ Paris Diderot | Williams Coll | Univ Hawaii | Fdn Bruno Kessler | Inst High Energy Phys | INFN Bologna | Univ Enna Kore | Univ Alberta | Fermilab Natl Accelerator Lab | Belgorod Natl Res Univ | Joint Inst Nucl Res | Univ Birmingham | INFN Roma Tre | Virginia Tech | Temple Univ | Univ Liverpool | Univ Warwick | Univ Lancaster | Budker Inst Nucl Phys | INFN Lab Nazl Sud | Univ Massachusetts | Univ Manchester | Univ Houston | Univ Edinburgh | Politecn Torino | Univ Calif Los Angeles | Univ Calif Riverside | Ft Lewis Coll

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Abstract
The activation of materials due to exposure to cosmic rays may become an important background source for experiments investigating rare event phenomena. DarkSide-20k, currently under construction at the Laboratori Nazionali del Gran Sasso, is a direct detection experiment for galactic dark matter particles, using a two-phase liquid-argon Time Projection Chamber (TPC) filled with 49.7 tonnes (active mass) of Underground Argon (UAr) depleted in 39Ar. Despite the outstanding capability of discriminating ������/������ background in argon TPCs, this background must be considered because of induced dead time or accidental coincidences mimicking dark-matter signals and it is relevant for low-threshold electron-counting measurements. Here, the cosmogenic activity of relevant long-lived radioisotopes induced in the experiment has been estimated to set requirements and procedures during preparation of the experiment and to check that it is not dominant over primordial radioactivity; particular attention has been paid to the activation of the 120 t of UAr used in DarkSide-20k. Expected exposures above ground and production rates, either measured or calculated, have been considered in detail. From the simulated counting rates in the detector due to cosmogenic isotopes, it is concluded that activation in copper and stainless steel is not problematic. The activity of 39Ar induced during extraction, purification and transport on surface is evaluated to be 2.8% of the activity measured in UAr by DarkSide-50 experiment, which used the same underground source, and thus considered acceptable. Other isotopes in the UAr such as 37Ar and 3H are shown not to be relevant due to short half-life and assumed purification methods.
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Cosmogenic activation,Argon,Dark matter,Rare events
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要点】:本文研究了宇宙射线引起的材料激活对DarkSide-20k实验背景的影响,并提出了相应的处理方法。

方法】:通过计算和分析宇宙射线在实验材料中诱导的长寿命放射性同位素的激活情况,评估其对实验背景的影响。

实验】:实验使用49.7吨地下贫化氩(UAr)作为探测介质,研究了宇宙射线在地表和地下对UAr以及实验材料(如铜和不锈钢)的激活情况,数据集来源于DarkSide-50实验,结果显示39Ar的激活率为2.8%,其他同位素如37Ar和3H因半衰期短和净化方法的影响而不显著。