Your browser doesn't support javascript.
loading
First Direct Search for Inelastic Boosted Dark Matter with COSINE-100.
Ha, C; Adhikari, G; Adhikari, P; Barbosa de Souza, E; Carlin, N; Choi, S; Djamal, M; Ezeribe, A 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
  • Ha C; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Adhikari G; Department of Physics, Sejong University, Seoul 05006, Republic of Korea.
  • Adhikari P; Department of Physics, Sejong University, Seoul 05006, Republic of Korea.
  • Barbosa de Souza E; 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.
  • 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; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Kim YH; Department of Physics, Sejong University, Seoul 05006, Republic of Korea.
  • Ko YJ; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Kudryavtsev VA; Korea Research Institute of Standards and Science, Daejeon 34113, Republic of Korea.
  • Lee HS; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Lee J; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Lee JY; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Lee MH; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Leonard DS; Department of Physics, Kyungpook National University, Daegu 41566, Republic of Korea.
  • Lynch WA; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Maruyama RH; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Mouton F; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Olsen SL; Department of Physics and Wright Laboratory, Yale University, New Haven, Connecticut 06520, USA.
  • Park BJ; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Park HK; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Park HS; IBS School, University of Science and Technology (UST), Daejeon 34113, Republic of Korea.
  • Park KS; Department of Accelerator Science, Korea University, Sejong 30019, Republic of Korea.
  • Pitta RLC; Korea Research Institute of Standards and Science, Daejeon 34113, Republic of Korea.
  • Prihtiadi H; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Ra SJ; Physics Institute, University of São Paulo, 05508-090, São Paulo, Brazil.
  • Rott C; Department of Physics, Bandung Institute of Technology, Bandung 40132, Indonesia.
  • Shin KA; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Scarff A; Department of Physics, Sungkyunkwan University, Suwon 16419, Republic of Korea.
  • Spooner NJC; Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Republic of Korea.
  • Thompson WG; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Yang L; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom.
  • Yu GH; Department of Physics and Wright Laboratory, Yale University, New Haven, Connecticut 06520, USA.
Phys Rev Lett ; 122(13): 131802, 2019 Apr 05.
Article em En | MEDLINE | ID: mdl-31012610
A search for inelastic boosted dark matter (IBDM) using the COSINE-100 detector with 59.5 days of data is presented. This relativistic dark matter is theorized to interact with the target material through inelastic scattering with electrons, creating a heavier state that subsequently produces standard model particles, such as an electron-positron pair. In this study, we search for this electron-positron pair in coincidence with the initially scattered electron as a signature for an IBDM interaction. No excess over the predicted background event rate is observed. Therefore, we present limits on IBDM interactions under various hypotheses, one of which allows us to explore an area of the dark photon parameter space that has not yet been covered by other experiments. This is the first experimental search for IBDM using a terrestrial detector.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Phys Rev Lett Ano de publicação: 2019 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Phys Rev Lett Ano de publicação: 2019 Tipo de documento: Article