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Search for solar axions with CsI(Tl) crystal detectors

Published 6 Apr 2016 in hep-ex, astro-ph.SR, and hep-ph | (1604.01825v3)

Abstract: The results of a search for solar axions from the Korea Invisible Mass Search (KIMS) experiment at the Yangyang Underground Laboratory are presented. Low-energy electron-recoil events would be produced by conversion of solar axions into electrons via the axio-electric effect in CsI(Tl) crystals. Using data from an exposure of 34,596 $\rm kg \cdot days$, we set a 90 \% confidence level upper limit on the axion-electron coupling, $g_{ae}$, of $1.39 \times 10{-11}$ for an axion mass less than 1 keV/$\rm c2$. This limit is lower than the indirect solar neutrino bound, and fully excludes QCD axions heavier than 0.48 eV/$\rm c2$ and 140.9 eV/$\rm c2$ for the DFSZ and KSVZ models respectively.

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