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First result of the experimental search for the 9.4 keV solar axion reactions with 83Kr in the copper proportional counter

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Title
First result of the experimental search for the 9.4 keV solar axion reactions with 83Kr in the copper proportional counter
Author(s)
Gavrilyuk Y.M.; Gangapshev A.M.; Derbin A.V.; Kazalov V.V.; Kim H.J.; Y.D. Kim; 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.
Publication Date
2015-03
Journal
PHYSICS OF PARTICLES AND NUCLEI, v.46, no.2, pp.152 - 156
Publisher
MAIK NAUKA/INTERPERIODICA/SPRINGER
Abstract
The experimental search for solar hadronic axions is started at the Baksan Neutrino Observatory of the Institute for Nuclear Researches of Russian Academy of Science (BNO INR RAS). It is assumed that axions are created in the Sun during M1 transition between the first thermally excited level at 9.4 keV and the ground state in 83Kr. The experiment is based on axion detection via resonant absorption process by the same nucleus in the detector. The big copper proportional counter filled with krypton is used to detect signals from axions. The experimental setup is situated in the deep underground low background laboratory. No evidence of axion detection were found after the 26.5 days data collection. Resulting new upper limit on axion mass is mA ≤ 130 eV at 95% C.L. © 2015, Pleiades Publishing, Ltd
URI
https://pr.ibs.re.kr/handle/8788114/1709
ISSN
1063-7796
Appears in Collections:
Center for Underground Physics(지하실험 연구단) > Journal Papers (저널논문)
Files in This Item:
Solar Axion YDKim 2015.pdfDownload

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