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A search for solar axion induced signals with COSINE-100
- Authors
- Adhikari, P.; Adhikari, G.; 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.; Rott, C.; Shin, K. A.; Scarff, A.; Spooner, N. J. C.; Thompsonb, W. G.; Yang, L.; Yu, G. H.
- Issue Date
- 1월-2020
- Publisher
- ELSEVIER
- Keywords
- Solar axion; COSINE-100; Dark matter
- Citation
- ASTROPARTICLE PHYSICS, v.114, pp.101 - 106
- Indexed
- SCIE
SCOPUS
- Journal Title
- ASTROPARTICLE PHYSICS
- Volume
- 114
- Start Page
- 101
- End Page
- 106
- ISSN
- 0927-6505
- Abstract
- We present results from a search for solar axions with the COSINE-100 experiment. We find no evidence of solar axion events from a data-set of 6,303.9 kg . days exposure and set a 90% confidence level upper limit on the axion-electron coupling, g(ae), of 1.70 x 10(-11) for an axion mass less than 1 keV/c(2). This limit excludes QCD axions heavier than 0.59 eV/c(2) in the DFSZ model and 1681 eV/c(2) in the KSVZ model. (C) 2019 Elsevier B.V. All rights reserved.
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