New limits on the resonant absorption of solar axions obtained with a 
$^\mathbf{169}$Tm-containing cryogenic detector

Abdelhameed, A.H.; Bakhlanov, S.V.; Bauer, P.; Bento, A.; Bertoldo, E.; Canonica, L.; Derbin, A.V.; Drachnev, I.S.; Ferreiro Iachellini, N.; Fuchs, D.; Hauff, D.; Laubenstein, M.; Lis, D.A.; Lomskaya, I.S.; Mancuso, M.; Muratova, V.N.; Nagorny, S.; Nisi, S.; Petricca, F.; Proebst, F.; Rothe, J.; Ryabchenkov, V.V.; Sarkisov, S.E.; Semenov, D.A.; Subbotin, K.A.; Trushin, M .V.; Unzhakov, E.V.; Zharikov, E.V.

doi:10.1140/epjc/s10052-020-7943-5

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Journal Article

New limits on the resonant absorption of solar axions obtained with a $^\mathbf{169}$Tm-containing cryogenic detector

MPS-Authors

Abdelhameed, A.H.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Bakhlanov, S.V.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Bauer, P.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Bento, A.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Bertoldo, E.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Canonica, L.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Derbin, A.V.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Drachnev, I.S.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Ferreiro Iachellini, N.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Fuchs, D.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Hauff, D.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Laubenstein, M.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Lis, D.A.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Lomskaya, I.S.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Mancuso, M.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Muratova, V.N.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Nagorny, S.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Nisi, S.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Petricca, F.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Proebst, F.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Rothe, J.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Ryabchenkov, V.V.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Sarkisov, S.E.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Semenov, D.A.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Subbotin, K.A.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Trushin, M .V.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Unzhakov, E.V.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Zharikov, E.V.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

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Citation

Abdelhameed, A., Bakhlanov, S., Bauer, P., Bento, A., Bertoldo, E., Canonica, L., et al. (2020). New limits on the resonant absorption of solar axions obtained with a $^\mathbf{169}$Tm-containing cryogenic detector. European Physical Journal C, 80, 376. doi:10.1140/epjc/s10052-020-7943-5.

Cite as: https://hdl.handle.net/21.11116/0000-0008-1BB7-C

Abstract

A search for resonant absorption of solar axions by $^{169}\mathrm{Tm}$ nuclei was carried out. A newly developed approach involving low-background cryogenic bolometer based on $\mathrm{Tm}_{3} \mathrm{Al}_{5} \mathrm{O}_{12}$ crystal was used that allowed for significant improvement of sensitivity in comparison with previous $^{169}\mathrm{Tm}$ based experiments. The measurements performed with \unit[$8.18$]{g} crystal during \unit[$6.6$]{days} exposure yielded the following limits on axion couplings: $|g_{A\gamma} (g_{AN}^0 + g_{AN}^3) \leq \unit[1.44 \times 10^{-14}]{GeV^{-1}}$ and $|g_{Ae} (g_{AN}^0 + g_{AN}^3) \leq 2.81 \times 10^{-16}$.