Abstract
Axions with an energy of 9.4 keV emitted in the M1 transition of 83Kr nuclei in the Sun have been sought in the resonance absorption reaction A + 83Kr → 83Kr* → 83Kr + γ, e (9.4 keV). A proportional gas chamber filled with krypton and placed in a low-background setup at the underground laboratory of the Baksan neutrino observatory was used to detect γ-ray photons and electrons appearing after the decay of a nuclear level. As a result, a new constraint has been determined on the isoscalar and isovector coupling constants of the axion with nucleons: |g 3 AN – g 0 AN | ≤ 1.29 × 10–6. This constraint results in the following new bound on the mass of the axion in the hadronic axion model: m A ≤ 100 eV (95% C.L.).
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Original Russian Text © Yu.M. Gavrilyuk, A.N. Gangapshev, A.V. Derbin, I.S. Drachnev, V.V. Kazalov, V.V. Kobychev, V.V. Kuz’minov, V.N. Muratova, S.I. Panasenko, S.S. Ratkevich, D.A. Semenov, D.A. Tekueva, E.V. Unzhakov, S.P. Yakimenko, 2015, published in Pis’ma v Zhurnal Eksperimental’noi i Teoreticheskoi Fiziki, 2015, Vol. 101, No. 10, pp. 739–745.
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Gavrilyuk, Y.M., Gangapshev, A.N., Derbin, A.V. et al. New experiment on search for the resonance absorption of solar axion emitted in the M1 transition of 83Kr nuclei. Jetp Lett. 101, 664–669 (2015). https://doi.org/10.1134/S0021364015100069
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DOI: https://doi.org/10.1134/S0021364015100069