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

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

doi:10.1134/S1063779615020094

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

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

Research output: Contribution to journal › Article › peer-review

5 Scopus citations

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 m_A ≤ 130 eV at 95% C.L.

Original language	English
Pages (from-to)	152-156
Number of pages	5
Journal	Physics of Particles and Nuclei
Volume	46
Issue number	2
DOIs	https://doi.org/10.1134/S1063779615020094
State	Published - 2015

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Gavrilyuk, Y. M., Gangapshev, A. M., Derbin, A. V., 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. (2015). First result of the experimental search for the 9.4 keV solar axion reactions with ⁸³Kr in the copper proportional counter. Physics of Particles and Nuclei, 46(2), 152-156. https://doi.org/10.1134/S1063779615020094

@article{0f2b2859fc86460bb277140b5af85976,

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

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.",

author = "Gavrilyuk, \{Yu M.\} and Gangapshev, \{A. M.\} and Derbin, \{A. V.\} and Kazalov, \{V. V.\} and Kim, \{H. J.\} and Kim, \{Y. D.\} and Kobychev, \{V. V.\} and Kuzminov, \{V. V.\} and Luqman Ali and Muratova, \{V. N.\} and Panasenko, \{S. I.\} and Ratkevich, \{S. S.\} and Semenov, \{D. A.\} and Tekueva, \{D. A.\} and Yakimenko, \{S. P.\} and Unzhakov, \{E. V.\}",

note = "Publisher Copyright: {\textcopyright} 2015, Pleiades Publishing, Ltd.",

year = "2015",

doi = "10.1134/S1063779615020094",

language = "English",

volume = "46",

pages = "152--156",

journal = "Physics of Particles and Nuclei",

issn = "1063-7796",

publisher = "Pleiades Publishing",

number = "2",

}

Gavrilyuk, YM, Gangapshev, AM, Derbin, AV, Kazalov, VV, Kim, HJ, Kim, YD, Kobychev, VV, Kuzminov, VV, Ali, L, Muratova, VN, Panasenko, SI, Ratkevich, SS, Semenov, DA, Tekueva, DA, Yakimenko, SP & Unzhakov, EV 2015, 'First result of the experimental search for the 9.4 keV solar axion reactions with ⁸³Kr in the copper proportional counter', Physics of Particles and Nuclei, vol. 46, no. 2, pp. 152-156. https://doi.org/10.1134/S1063779615020094

TY - JOUR

T1 - First result of the experimental search for the 9.4 keV solar axion reactions with 83Kr in the copper proportional counter

AU - Gavrilyuk, Yu M.

AU - Gangapshev, A. M.

AU - Derbin, A. V.

AU - Kazalov, V. V.

AU - Kim, H. J.

AU - Kim, Y. D.

AU - Kobychev, V. V.

AU - Kuzminov, V. V.

AU - Ali, Luqman

AU - Muratova, V. N.

AU - Panasenko, S. I.

AU - Ratkevich, S. S.

AU - Semenov, D. A.

AU - Tekueva, D. A.

AU - Yakimenko, S. P.

AU - Unzhakov, E. V.

PY - 2015

Y1 - 2015

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/84924762752

U2 - 10.1134/S1063779615020094

DO - 10.1134/S1063779615020094

M3 - Article

AN - SCOPUS:84924762752

SN - 1063-7796

VL - 46

SP - 152

EP - 156

JO - Physics of Particles and Nuclei

JF - Physics of Particles and Nuclei

IS - 2

ER -

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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