New limit on the mass of 9.4-keV solar axions emitted in an M1 transition in $\mathrm{^{83}Kr}$ nuclei

Derbin, A. V.; Semenov, D. A.; Panasenko, S. I.; Ali, Luqman; Ratkevich, S. S.; Kuzminov, V. V.; Tekueva, D. A.; Kim, Y. D.; Unzhakov, E. V.; Muratova, V. N.; Yakimenko, S. P.; Kazalov, V. V.; Kobychev, V. V.; Gangapshev, A. M.; Kim, H. J.; Gavrilyuk, Yu. M.

Contribution to a conference proceedings/Contribution to a book

PUBDB-2016-05910

New limit on the mass of 9.4-keV solar axions emitted in an M1 transition in $\mathrm{^{83}Kr}$ nuclei

Derbin, A. V. ; Gangapshev, A. M. ; Gavrilyuk, Y. M. ; Kazalov, V. V. ; Kim, H. J. ; Kim, Y. D. ; Kobychev, V. V. ; Kuzminov, V. V. ; Ali, L. ; Muratova, V. N. ; Panasenko, S. I. ; Ratkevich, S. S. ; Semenov, D. A. ; Tekueva, D. A. ; Yakimenko, S. P. ; Unzhakov, E. V.

2014
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-935702-59-1

Derbin, A.V. "New limit on the mass of 9.4-keV solar axions emitted in an M1 transition in $^{83}$Kr nuclei" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
10th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2014, Geneva, Switzerland, 29 Jun 2014 - 4 Jul 2014 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 55-58 (2014) [10.3204/DESY-PROC-2014-03/derbin_alexander]

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2014-03/derbin_alexander

Abstract: A search for resonant absorption of the solar axion by $^{83}\rm{Kr}$ nuclei was performed using the proportional counter installed inside the low-background setup at the Baksan Neutrino Observatory. The obtained model independent upper limit on the combination of isoscalar and isovector axion-nucleon couplings $|g_3-g_0|\leq 1.69\times 10^{-6}$ allowed us to set the new upper limit on the hadronic axion mass of $m_{A}\leq 130$ eV (95\% C.L.) with the generally accepted values $S$=0.5 and $z$=0.56.

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