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 |
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Main Authors: | , , , , , , , , , , |
Format: | Journal Article |
Language: | English |
Published: |
Moscow
Pleiades Publishing
01-07-2022
Springer Nature B.V |
Subjects: | |
Online Access: | Get full text |
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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. |
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ISSN: | 0021-3640 1090-6487 |
DOI: | 10.1134/S0021364022601075 |