[논문]Study of cosmogenic radionuclides in the COSINE-100 NaI(Tl) detectors

Barbosa de Souza, E.; Park, B.J.; Adhikari, G.; Adhikari, P.; Carlin, N.; Choi, J.J.; Choi, S.; Djamal, M.; Ezeribe, A.C.; Ha, C.; Hahn, I.S.; Jeon, E.J.; Jo, J.H.; Kang, W.G.; 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, E.K.; Lee, H.S.; Lee, J.; Lee, J.Y.; Lee, M.H.; Lee, S.H.; Leonard, D.S.; Lynch, W.A.; Manzato, B.B.; Maruyama, R.H.; Neal, R.J.; Olsen, S.L.; 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.

doi:10.1016/j.astropartphys.2019.102390

[해외논문] Study of cosmogenic radionuclides in the COSINE-100 NaI(Tl) detectors 원문보기

Astroparticle physics, v.115, 2020년, pp.102390 -

Barbosa de Souza, E. (Department of Physics, Yale University) , Park, B.J. (Corresponding authors.) , Adhikari, G. (Department of Physics, Sejong University) , Adhikari, P. (Department of Physics, Sejong University) , Carlin, N. (Physics Institute, University of Sã) , Choi, J.J. (o Paulo) , Choi, S. (Department of Physics and Astronomy, Seoul National University) , Djamal, M. (Department of Physics and Astronomy, Seoul National University) , Ezeribe, A.C. (Department of Physics, Bandung Institute of Technology) , Ha, C. (Department of Physics and Astronomy, University of Sheffield) , Hahn, I.S. (Center for Underground Physics, Institute for Basic Science (IBS)) , Jeon, E.J. (Department of Science Education, Ewha Womans University) , Jo, J.H. (Corresponding authors.) , Kang, W.G. (Department of Physics, Yale University) , 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, E.K. , Lee, H.S. , Lee, J. , Lee, J.Y. , Lee, M.H. , Lee, S.H. , Leonard, D.S. , Lynch, W.A. , Manzato, B.B. , Maruyama, R.H. , Neal, R.J. , Olsen, S.L. , 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.

Abstract ▼ AI-Helper

Abstract COSINE-100 is a direct detection dark matter search experiment that uses a 106 kg array of eight NaI(Tl) crystals that are kept underground at the Yangyang Underground Laboratory to avoid cosmogenic activation of radioisotopes by cosmic rays. Even though the cosmogenic activity is declining with time, there are still significant background rates from the remnant nuclides. In this paper, we report measurements of cosmogenic isotope contaminations with less than one year half-lives that are based on extrapolations of the time dependent activities of their characteristic energy peaks to activity rates at the time the crystals were deployed underground. For longer-lived 109Cd ( T 1 / 2 = 1.27 y) and 22Na ( T 1 / 2 = 2.6 y), we investigate time correlations and coincidence events due to several emissions. The inferred sea-level production rates are compared with calculations based on the ACTIVIA and MENDL-2 model calculations and experimental data. The results from different approaches are in reasonable agreement with each other. For 3H, which has a long, 12.3 year half-life, we evaluated the activity levels and the exposure times that are in reasonable agreement with the time period estimated for each crystal’s exposure.

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