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Search for resonant absorption of solar axions emitted in M1-transitions in 83Kr nuclei: Second stage of the experiment

  • The International Session-Conference of SNP PSD RAS “Physics of Fundamental Interactions” April 12–15, 2016, Dubna, Russia
  • Session 9—Astroparticle physics
  • Published:
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Abstract

Axions with energies of 9.4 keV putatively produced in the Sun via an M1-transition in the 83Kr nucleus are searched for using the reaction of resonant absorption: A +83Kr →83Kr* →83Kr + γ, e (9.4 keV). The γ-quanta and electrons are detected with a proportional counter filled with krypton and placed in a low-background setup. A new upper limit on the axion–nucleon coupling constant is imposed: |g 3AN g 0AN |≤1.02 106. For the hadronic axion, this implies a new upper limit on the axion mass: m A ≤ 79eV at the 95% confidence level.

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Correspondence to A. M. Gangapshev.

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Original Russian Text © Yu.M. Gavrilyuk, A.M. Gangapshev, A.V. Derbin, V.V. Kazalov, V.V. Kuzminov, V.N. Muratova, S.I. Panasenko, S.S. Ratkevich, D.A. Tekueva, E.V. Unzhakov, S.P. Yakimenko, 2018, published in Fizika Elementarnykh Chastits i Atomnogo Yadra, 2018, Vol. 49, No. 1.

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Gavrilyuk, Y.M., Gangapshev, A.M., Derbin, A.V. et al. Search for resonant absorption of solar axions emitted in M1-transitions in 83Kr nuclei: Second stage of the experiment. Phys. Part. Nuclei 49, 94–96 (2018). https://doi.org/10.1134/S1063779618010136

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  • DOI: https://doi.org/10.1134/S1063779618010136

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