New limits on the resonant absorption of solar axions obtained with a $$^\mathbf {169}$$ 169 Tm-containing cryogenic detector
Autor: | A. H. Abdelhameed, S. V. Bakhlanov, P. Bauer, A. Bento, E. Bertoldo, L. Canonica, A. V. Derbin, I. S. Drachnev, N. Ferreiro Iachellini, D. Fuchs, D. Hauff, M. Laubenstein, D. A. Lis, I. S. Lomskaya, M. Mancuso, V. N. Muratova, S. Nagorny, S. Nisi, F. Petricca, F. Proebst, J. Rothe, V. V. Ryabchenkov, S. E. Sarkisov, D. A. Semenov, K. A. Subbotin, M. V. Trushin, E. V. Unzhakov, E. V. Zharikov |
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Jazyk: | angličtina |
Rok vydání: | 2020 |
Předmět: | |
Zdroj: | European Physical Journal C: Particles and Fields, Vol 80, Iss 5, Pp 1-7 (2020) |
Druh dokumentu: | article |
ISSN: | 1434-6044 1434-6052 |
DOI: | 10.1140/epjc/s10052-020-7943-5 |
Popis: | Abstract A search for resonant absorption of solar axions by $$^{169}\mathrm {Tm}$$ 169Tm nuclei was carried out. A newly developed approach involving low-background cryogenic bolometer based on $$\mathrm {Tm}_{3} \mathrm {Al}_{5} \mathrm {O}_{12}$$ Tm3Al5O12 crystal was used that allowed for significant improvement of sensitivity in comparison with previous $$^{169}\mathrm {Tm}$$ 169Tm based experiments. The measurements performed with 8.18 g crystal during 6.6 days exposure yielded the following limits on axion couplings: $$|g_{A\gamma } (g_{AN}^0 + g_{AN}^3) \le 1.44 \times 10^{-14}\,{{\mathrm{GeV}}^{-1}}$$ |gAγ(gAN0+gAN3)≤1.44×10-14GeV-1 and $$|g_{Ae} (g_{AN}^0 + g_{AN}^3) \le 2.81 \times 10^{-16}$$ |gAe(gAN0+gAN3)≤2.81×10-16 . |
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