New Constraints on the Axion–Electron Coupling Constant for Solar Axions

The resonant excitation of the 83 Kr first excited nuclear level ( E = 9.4 keV) by solar axions whose fluxes depend on the axion–electron coupling constant g Ae is sought. The γ- and X-ray photons and the conversion and Auger electrons from the excited-level relaxation are detected with a gas propor...

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Published in:JETP letters Vol. 116; no. 1; pp. 11 - 17
Main Authors: Gavrilyuk, Yu. M., Gangapshev, A. N., Derbin, A. V., Drachnev, I. S., Kazalov, V. V., Kuzminov, V. V., Mikulich, M. S., Muratova, V. N., Tekueva, D. A., Unzhakov, E. V., Yakimenko, S. P.
Format: Journal Article
Language:English
Published: Moscow Pleiades Publishing 01-07-2022
Springer Nature B.V
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Summary:The resonant excitation of the 83 Kr first excited nuclear level ( E = 9.4 keV) by solar axions whose fluxes depend on the axion–electron coupling constant g Ae is sought. The γ- and X-ray photons and the conversion and Auger electrons from the excited-level relaxation are detected with a gas proportional counter of a low-background detector in the underground Baksan Neutrino Observatory (Institute for Nuclear Research, Russian Academy of Sciences). As a result, a new constraint ≤ 1.50 × 10 –17 (90% C.L.) has been obtained for the axion–electron and axion–nucleon coupling constants, which corresponds to new constraints on the axion mass m A ≤ 320 eV and m A ≤ 4.6 eV in the KSVZ and DFSZ axion models, respectively.
ISSN:0021-3640
1090-6487
DOI:10.1134/S0021364022601075