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Search for a Dark Matter-Induced Annual Modulation Signal in NaI(Tl) with the COSINE-100 Experiment.
Adhikari, G; Adhikari, P; de Souza, E Barbosa; Carlin, N; Choi, S; Djamal, M; Ezeribe, A C; Ha, C; Hahn, I S; Jeon, E J; Jo, J H; Joo, H W; Kang, W G; Kang, W; Kauer, M; Kim, G S; Kim, H; Kim, H J; Kim, K W; Kim, N Y; Kim, S K; Kim, Y D; Kim, Y H; Ko, Y J; 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, B J; Park, H K; Park, H S; Park, K S; Pitta, R L C; Prihtiadi, H; Ra, S J; Rott, C; Shin, K A; Scarff, A; Spooner, N J C; Thompson, W G; Yang, L; Yu, G H.
Afiliação
  • Adhikari G; Department of Physics, Sejong University, Seoul 05006, Republic of Korea.
  • Adhikari P; Department of Physics, Sejong University, Seoul 05006, Republic of Korea.
  • de Souza EB; Department of Physics and Wright Laboratory, Yale University, New Haven, Connecticut 06520, USA.
  • Carlin N; Physics Institute, University of São Paulo, 05508-090, São Paulo, Brazil.
  • Choi S; Department of Physics and Astronomy, Seoul National University, Seoul 08826, Republic of Korea.
  • Djamal M; Department of Physics, Bandung Institute of Technology, Bandung 40132, Indonesia.
  • Ezeribe AC; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Ha C; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Hahn IS; Department of Science Education, Ewha Womans University, Seoul 03760, Republic of Korea.
  • Jeon EJ; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Jo JH; Department of Physics and Wright Laboratory, Yale University, New Haven, Connecticut 06520, USA.
  • Joo HW; Department of Physics and Astronomy, Seoul National University, Seoul 08826, Republic of Korea.
  • Kang WG; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Kang W; Department of Physics, Sungkyunkwan University, Suwon 16419, Republic of Korea.
  • Kauer M; Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA.
  • Kim GS; Department of Physics, Kyungpook National University, Daegu 41566, Republic of Korea.
  • Kim H; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Kim HJ; Department of Physics, Kyungpook National University, Daegu 41566, Republic of Korea.
  • Kim KW; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Kim NY; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Kim SK; Department of Physics and Astronomy, Seoul National University, Seoul 08826, Republic of Korea.
  • Kim YD; Department of Physics, Sejong University, Seoul 05006, Republic of Korea.
  • Kim YH; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Ko YJ; IBS School, University of Science and Technology (UST), Daejeon 34113, Republic of Korea.
  • Kudryavtsev VA; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Lee HS; IBS School, University of Science and Technology (UST), Daejeon 34113, Republic of Korea.
  • Lee J; Korea Research Institute of Standards and Science, Daejeon 34113, Republic of Korea.
  • Lee JY; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Lee MH; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Leonard DS; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Lynch WA; IBS School, University of Science and Technology (UST), Daejeon 34113, Republic of Korea.
  • Maruyama RH; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Mouton F; Department of Physics, Kyungpook National University, Daegu 41566, Republic of Korea.
  • Olsen SL; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Park BJ; IBS School, University of Science and Technology (UST), Daejeon 34113, Republic of Korea.
  • Park HK; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Park HS; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Park KS; Department of Physics and Wright Laboratory, Yale University, New Haven, Connecticut 06520, USA.
  • Pitta RLC; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Prihtiadi H; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Ra SJ; IBS School, University of Science and Technology (UST), Daejeon 34113, Republic of Korea.
  • Rott C; Department of Accelerator Science, Korea University, Sejong 30019, Republic of Korea.
  • Shin KA; Korea Research Institute of Standards and Science, Daejeon 34113, Republic of Korea.
  • Scarff A; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Spooner NJC; Physics Institute, University of São Paulo, 05508-090, São Paulo, Brazil.
  • Thompson WG; Department of Physics, Bandung Institute of Technology, Bandung 40132, Indonesia.
  • Yang L; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Yu GH; Department of Physics, Sungkyunkwan University, Suwon 16419, Republic of Korea.
Phys Rev Lett ; 123(3): 031302, 2019 Jul 19.
Article em En | MEDLINE | ID: mdl-31386435
ABSTRACT
We present new constraints on the dark matter-induced annual modulation signal using 1.7 years of COSINE-100 data with a total exposure of 97.7 kg yr. The COSINE-100 experiment, consisting of 106 kg of NaI(Tl) target material, is designed to carry out a model-independent test of DAMA/LIBRA's claim of WIMP discovery by searching for the same annual modulation signal using the same NaI(Tl) target. The crystal data show a 2.7 cpd/kg/keV background rate on average in the 2-6 keV energy region of interest. Using a χ-squared minimization method we observe best fit values for modulation amplitude and phase of 0.0092±0.0067 cpd/kg/keV and 127.2±45.9 d, respectively.

Texto completo: 1 Bases de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2019 Tipo de documento: Article

Texto completo: 1 Bases de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2019 Tipo de documento: Article