COSINE-100的NaI(Tl)晶体中的α背景

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
G. Adhikari , N. Carlin , D.F.F.S. Cavalcante , J.Y. Cho , J.J. Choi , S. Choi , A.C. Ezeribe , L.E. França , C. Ha , I.S. Hahn , S.J. Hollick , E.J. Jeon , H.W. Joo , W.G. Kang , M. Kauer , B.H. Kim , H.J. Kim , J. Kim , K.W. Kim , S.H. Kim , G.H. Yu
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引用次数: 0

摘要

COSINE-100 是一项暗物质直接探测实验,以 106 千克 NaI(Tl)为目标物质。210Pb 和子同位素是 WIMP 感兴趣区域的主要背景,通过 β 衰变和 α 衰变进行探测。对 α 频道的分析补充了在β/γ 频道观测到的背景模型。我们介绍了 COSINE-100 NaI(Tl)晶体的淬灭因子测量结果、蒙特卡罗模拟结果以及α衰变成分的活性定量。数据有力地表明,α衰变可能经历了两种可能的淬灭因子,但还需要进一步研究。拟合结果与独立测量结果一致,并提高了对 COSINE-100 背景的整体认识。此外,216Po 的半衰期被测量为 143.4±1.2 毫秒,这与目前大多数测量结果一致,而且更加精确。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Alpha backgrounds in NaI(Tl) crystals of COSINE-100

COSINE-100 is a dark matter direct detection experiment with 106 kg NaI(Tl) as the target material. 210Pb and daughter isotopes are a dominant background in the WIMP region of interest and are detected via β decay and α decay. Analysis of the α channel complements the background model as observed in the β/γ channel. We present the measurement of the quenching factors and Monte Carlo simulation results and activity quantification of the α decay components of the COSINE-100 NaI(Tl) crystals. The data strongly indicate that the α decays probabilistically undergo two possible quenching factors but require further investigation. The fitted results are consistent with independent measurements and improve the overall understanding of the COSINE-100 backgrounds. Furthermore, the half-life of 216Po has been measured to be 143.4±1.2  ms, which is consistent with and more precise than most current measurements.

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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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