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
{"title":"COSINE-100的NaI(Tl)晶体中的α背景","authors":"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","doi":"10.1016/j.astropartphys.2024.102945","DOIUrl":null,"url":null,"abstract":"<div><p>COSINE-100 is a dark matter direct detection experiment with 106<!--> <!-->kg NaI(Tl) as the target material. <sup>210</sup>Pb and daughter isotopes are a dominant background in the WIMP region of interest and are detected via <span><math><mi>β</mi></math></span> decay and <span><math><mi>α</mi></math></span> decay. Analysis of the <span><math><mi>α</mi></math></span> channel complements the background model as observed in the <span><math><mi>β</mi></math></span>/<span><math><mi>γ</mi></math></span> channel. We present the measurement of the quenching factors and Monte Carlo simulation results and activity quantification of the <span><math><mi>α</mi></math></span> decay components of the COSINE-100 NaI(Tl) crystals. The data strongly indicate that the <span><math><mi>α</mi></math></span> 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 <sup>216</sup>Po has been measured to be <span><math><mrow><mn>143</mn><mo>.</mo><mn>4</mn><mspace></mspace><mo>±</mo><mspace></mspace><mn>1</mn><mo>.</mo><mn>2</mn></mrow></math></span> <!--> <!-->ms, which is consistent with and more precise than most current measurements.</p></div>","PeriodicalId":55439,"journal":{"name":"Astroparticle Physics","volume":"158 ","pages":"Article 102945"},"PeriodicalIF":4.2000,"publicationDate":"2024-02-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Alpha backgrounds in NaI(Tl) crystals of COSINE-100\",\"authors\":\"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\",\"doi\":\"10.1016/j.astropartphys.2024.102945\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>COSINE-100 is a dark matter direct detection experiment with 106<!--> <!-->kg NaI(Tl) as the target material. <sup>210</sup>Pb and daughter isotopes are a dominant background in the WIMP region of interest and are detected via <span><math><mi>β</mi></math></span> decay and <span><math><mi>α</mi></math></span> decay. Analysis of the <span><math><mi>α</mi></math></span> channel complements the background model as observed in the <span><math><mi>β</mi></math></span>/<span><math><mi>γ</mi></math></span> channel. We present the measurement of the quenching factors and Monte Carlo simulation results and activity quantification of the <span><math><mi>α</mi></math></span> decay components of the COSINE-100 NaI(Tl) crystals. The data strongly indicate that the <span><math><mi>α</mi></math></span> 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 <sup>216</sup>Po has been measured to be <span><math><mrow><mn>143</mn><mo>.</mo><mn>4</mn><mspace></mspace><mo>±</mo><mspace></mspace><mn>1</mn><mo>.</mo><mn>2</mn></mrow></math></span> <!--> <!-->ms, which is consistent with and more precise than most current measurements.</p></div>\",\"PeriodicalId\":55439,\"journal\":{\"name\":\"Astroparticle Physics\",\"volume\":\"158 \",\"pages\":\"Article 102945\"},\"PeriodicalIF\":4.2000,\"publicationDate\":\"2024-02-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astroparticle Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0927650524000227\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astroparticle Physics","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0927650524000227","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
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 decay and decay. Analysis of the channel complements the background model as observed in the / channel. We present the measurement of the quenching factors and Monte Carlo simulation results and activity quantification of the decay components of the COSINE-100 NaI(Tl) crystals. The data strongly indicate that the 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 ms, which is consistent with and more precise than most current measurements.
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.