학술논문
New limits on the resonant absorption of solar axions obtained with a $^{169}$Tm-containing cryogenic detector
Document Type
Working Paper
Author
Abdelhameed, A. H.; Bakhlanov, S. V.; Bauer, P.; Bento, A.; Bertoldo, E.; Canonica, L.; Derbin, A. V.; Drachnev, I. S.; Iachellini, N. Ferreiro; 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.
Source
Subject
Language
Abstract
A search for resonant absorption of solar axions by $^{169}$Tm nuclei was carried out. A newly developed approach involving low-background cryogenic bolometer based on Tm$_3$Al$_5$O$_{12}$ crystal was used that allowed for significant improvement of sensitivity in comparison with previous $^{169}$Tm based experiments. The measurements performed with $8.18$ g crystal during $6.6$ days exposure yielded the following limits on axion couplings: $|g_{A\gamma} (g_{AN}^0 + g_{AN}^3) \leq 1.44 \times 10^{-14}$ GeV$^{-1}$ and $|g_{Ae} (g_{AN}^0 + g_{AN}^3) \leq 2.81 \times 10^{-16}$.
Comment: 7 pages, 5 figures
Comment: 7 pages, 5 figures