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Background model for the NaI(Tl) crystals in COSINE-100.
Adhikari, P; Adhikari, G; Souza, E Barbosa de; Carlin, N; Choi, S; Choi, W Q; Djamal, M; Ezeribe, A C; Ha, C; Hahn, I S; Hubbard, A J F; Jeon, E J; Jo, J H; Joo, H W; Kang, W G; Kauer, M; Kang, W S; Kim, B H; Kim, H; Kim, H J; Kim, K W; Kim, M C; Kim, N Y; Kim, S K; Kim, Y D; Kim, Y H; Kudryavtsev, V A; Lee, H S; Lee, J; Lee, J Y; Lee, M H; Leonard, D S; Lynch, W A; Maruyama, R H; Mouton, F; Olsen, S L; Park, H K; Park, H S; Park, J S; Park, K S; Pettus, W; Prihtiadi, H; Ra, S; Rott, C; Scarff, A; Spooner, N J C; Thompson, W G; Yang, L; Yong, S H.
Afiliação
  • Adhikari P; 1Department of Physics and Astronomy, Sejong University, Seoul, 05006 South Korea.
  • Adhikari G; 1Department of Physics and Astronomy, Sejong University, Seoul, 05006 South Korea.
  • Souza EB; 2Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520 USA.
  • Carlin N; 3Physics Institute, University of São Paulo, São Paulo, 05508-090 Brazil.
  • Choi S; 4Department of Physics and Astronomy, Seoul National University, Seoul, 08826 Republic of Korea.
  • Choi WQ; Korea Institue of Science and Technology Information, Daejeon, 34141 Republic of Korea.
  • Djamal M; 6Department of Physics, Bandung Institute of Technology, Bandung, 40132 Indonesia.
  • Ezeribe AC; 7Department of Physics and Astronomy, University of Sheffield, Sheffield, S3 7RH UK.
  • Ha C; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Hahn IS; 9Department of Science Education, Ewha Womans University, Seoul, 03760 Republic of Korea.
  • Hubbard AJF; 2Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520 USA.
  • Jeon EJ; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Jo JH; 2Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520 USA.
  • Joo HW; 4Department of Physics and Astronomy, Seoul National University, Seoul, 08826 Republic of Korea.
  • Kang WG; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Kauer M; 11Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI 53706 USA.
  • Kang WS; 10Department of Physics, Sungkyunkwan University, Seoul, 16419 Republic of Korea.
  • Kim BH; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Kim H; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Kim HJ; 12Department of Physics, Kyungpook National University, Daegu, 41566 Republic of Korea.
  • Kim KW; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Kim MC; 10Department of Physics, Sungkyunkwan University, Seoul, 16419 Republic of Korea.
  • Kim NY; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Kim SK; 4Department of Physics and Astronomy, Seoul National University, Seoul, 08826 Republic of Korea.
  • Kim YD; 1Department of Physics and Astronomy, Sejong University, Seoul, 05006 South Korea.
  • Kim YH; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Kudryavtsev VA; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Lee HS; 13Korea Research Institute of Standards and Science, Daejeon, 34113 Republic of Korea.
  • Lee J; 7Department of Physics and Astronomy, University of Sheffield, Sheffield, S3 7RH UK.
  • Lee JY; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Lee MH; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Leonard DS; 4Department of Physics and Astronomy, Seoul National University, Seoul, 08826 Republic of Korea.
  • Lynch WA; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Maruyama RH; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Mouton F; 7Department of Physics and Astronomy, University of Sheffield, Sheffield, S3 7RH UK.
  • Olsen SL; 2Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520 USA.
  • Park HK; 7Department of Physics and Astronomy, University of Sheffield, Sheffield, S3 7RH UK.
  • Park HS; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Park JS; 15Department of Accelerator Science, Graduate School, Korea University, Sejong, 30019 South Korea.
  • Park KS; 13Korea Research Institute of Standards and Science, Daejeon, 34113 Republic of Korea.
  • Pettus W; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Prihtiadi H; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Ra S; 2Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520 USA.
  • Rott C; 6Department of Physics, Bandung Institute of Technology, Bandung, 40132 Indonesia.
  • Scarff A; 8Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126 Republic of Korea.
  • Spooner NJC; 10Department of Physics, Sungkyunkwan University, Seoul, 16419 Republic of Korea.
  • Thompson WG; 7Department of Physics and Astronomy, University of Sheffield, Sheffield, S3 7RH UK.
  • Yang L; 7Department of Physics and Astronomy, University of Sheffield, Sheffield, S3 7RH UK.
  • Yong SH; 2Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520 USA.
Eur Phys J C Part Fields ; 78(6): 490, 2018.
Article em En | MEDLINE | ID: mdl-30956554
ABSTRACT
The COSINE-100 dark matter search experiment is an array of NaI(Tl) crystal detectors located in the Yangyang Underground Laboratory (Y2L). To understand measured backgrounds in the NaI(Tl) crystals we have performed Monte Carlo simulations using the Geant4 toolkit and developed background models for each crystal that consider contributions from both internal and external sources, including cosmogenic nuclides. The background models are based on comparisons of measurement data with Monte Carlo simulations that are guided by a campaign of material assays and are used to evaluate backgrounds and identify their sources. The average background level for the six crystals (70 kg total mass) that are studied is 3.5 counts/day/keV/kg in the (2-6) keV energy interval. The dominant contributors in this energy region are found to be 210 Pb and 3 H.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2018 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2018 Tipo de documento: Article