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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.
Scar, A.
Spooner, N. J. C.
Thompson, W. G.
Yang, L.
Yu, G. H.
Publication Year :
2019

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$\cdot$days exposure and set a 90\,\% confidence level upper limit on the axion-electron coupling, $g_{ae}$, at 1.70~$\times$~$10^{-11}$ 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 168.1\,eV/c$^2$ in the KSVZ model.<br />Comment: 7 pages, 8 figures

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1904.06860
Document Type :
Working Paper
Full Text :
https://doi.org/10.1016/j.astropartphys.2019.07.004