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Search for solar axions produced by Compton process and bremsstrahlung using the resonant absorption and axioelectric effect (1312.0187v1)

Published 1 Dec 2013 in hep-ex, astro-ph.SR, and hep-ph

Abstract: The search for resonant absorption of Compton and bremsstrahlung solar axions by ${169}$Tm nuclei have been performed. Such an absorption should lead to the excitation of low-lying nuclear energy level: $A+{169}$Tm $\rightarrow {169}$Tm$*$ $\rightarrow {169}$Tm $+ \gamma$ (8.41 keV). Additionally the axio-electric effect in silicon atoms is sought. The axions are detected using a Si(Li) detectors placed in a low-background setup. As a result, a new model independent restrictions on the axion-electron and the axion-nucleon coupling: $g_{Ae}\times|g0_{AN}+ g3_{AN}|\leq 2.1\times10{-14}$ and the axion-electron coupling constant: $|g_{Ae}| \leq 2.2\times 10{-10}$ has been obtained. The limits leads to the bounds $m_{A}\leq$ 7.9 eV and $m_{A}\leq$ 1.3 keV for the mass of the axion in the DFSZ and KSVZ models, respectively ($90\%$ C.L.).

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