New experiment on search for the resonance absorption of solar axion emitted in the M1 transition of 83Kr nuclei
Axions with an energy of 9.4 keV emitted in the M 1 transition of 83 Kr nuclei in the Sun have been sought in the resonance absorption reaction A + 83 Kr → 83 Kr* → 83 Kr + γ, e (9.4 keV). A proportional gas chamber filled with krypton and placed in a low-background setup at the underground laborato...
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| Veröffentlicht in: | JETP letters 2015-05, Vol.101 (10), p.664-669 |
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| creator | Gavrilyuk, Yu. M. Gangapshev, A. N. Derbin, A. V. Drachnev, I. S. Kazalov, V. V. Kobychev, V. V. Kuz’minov, V. V. Muratova, V. N. Panasenko, S. I. Ratkevich, S. S. Semenov, D. A. Tekueva, D. A. Unzhakov, E. V. Yakimenko, S. P. |
| description | Axions with an energy of 9.4 keV emitted in the
M
1 transition of
83
Kr nuclei in the Sun have been sought in the resonance absorption reaction
A
+
83
Kr →
83
Kr* →
83
Kr + γ,
e
(9.4 keV). A proportional gas chamber filled with krypton and placed in a low-background setup at the underground laboratory of the Baksan neutrino observatory was used to detect γ-ray photons and electrons appearing after the decay of a nuclear level. As a result, a new constraint has been determined on the isoscalar and isovector coupling constants of the axion with nucleons: |
g
AN
3
–
g
AN
0
| ≤ 1.29 × 10
–6
. This constraint results in the following new bound on the mass of the axion in the hadronic axion model:
m
A
≤ 100 eV (95% C.L.). |
| doi_str_mv | 10.1134/S0021364015100069 |
| format | Article |
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M
1 transition of
83
Kr nuclei in the Sun have been sought in the resonance absorption reaction
A
+
83
Kr →
83
Kr* →
83
Kr + γ,
e
(9.4 keV). A proportional gas chamber filled with krypton and placed in a low-background setup at the underground laboratory of the Baksan neutrino observatory was used to detect γ-ray photons and electrons appearing after the decay of a nuclear level. As a result, a new constraint has been determined on the isoscalar and isovector coupling constants of the axion with nucleons: |
g
AN
3
–
g
AN
0
| ≤ 1.29 × 10
–6
. This constraint results in the following new bound on the mass of the axion in the hadronic axion model:
m
A
≤ 100 eV (95% C.L.).</description><identifier>ISSN: 0021-3640</identifier><identifier>EISSN: 1090-6487</identifier><identifier>DOI: 10.1134/S0021364015100069</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Atomic ; Biological and Medical Physics ; Biophysics ; Fields ; Molecular ; Nuclei ; Optical and Plasma Physics ; Particle and Nuclear Physics ; Particles ; Physics ; Physics and Astronomy ; Quantum Information Technology ; Solid State Physics ; Spintronics</subject><ispartof>JETP letters, 2015-05, Vol.101 (10), p.664-669</ispartof><rights>Pleiades Publishing, Inc. 2015</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c1999-b0d8c30ad277ba88eaf67e7e98d4c2004b62024668721942a90b454207f15b2d3</citedby><cites>FETCH-LOGICAL-c1999-b0d8c30ad277ba88eaf67e7e98d4c2004b62024668721942a90b454207f15b2d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0021364015100069$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0021364015100069$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Gavrilyuk, Yu. M.</creatorcontrib><creatorcontrib>Gangapshev, A. N.</creatorcontrib><creatorcontrib>Derbin, A. V.</creatorcontrib><creatorcontrib>Drachnev, I. S.</creatorcontrib><creatorcontrib>Kazalov, V. V.</creatorcontrib><creatorcontrib>Kobychev, V. V.</creatorcontrib><creatorcontrib>Kuz’minov, V. V.</creatorcontrib><creatorcontrib>Muratova, V. N.</creatorcontrib><creatorcontrib>Panasenko, S. I.</creatorcontrib><creatorcontrib>Ratkevich, S. S.</creatorcontrib><creatorcontrib>Semenov, D. A.</creatorcontrib><creatorcontrib>Tekueva, D. A.</creatorcontrib><creatorcontrib>Unzhakov, E. V.</creatorcontrib><creatorcontrib>Yakimenko, S. P.</creatorcontrib><title>New experiment on search for the resonance absorption of solar axion emitted in the M1 transition of 83Kr nuclei</title><title>JETP letters</title><addtitle>Jetp Lett</addtitle><description>Axions with an energy of 9.4 keV emitted in the
M
1 transition of
83
Kr nuclei in the Sun have been sought in the resonance absorption reaction
A
+
83
Kr →
83
Kr* →
83
Kr + γ,
e
(9.4 keV). A proportional gas chamber filled with krypton and placed in a low-background setup at the underground laboratory of the Baksan neutrino observatory was used to detect γ-ray photons and electrons appearing after the decay of a nuclear level. As a result, a new constraint has been determined on the isoscalar and isovector coupling constants of the axion with nucleons: |
g
AN
3
–
g
AN
0
| ≤ 1.29 × 10
–6
. This constraint results in the following new bound on the mass of the axion in the hadronic axion model:
m
A
≤ 100 eV (95% C.L.).</description><subject>Atomic</subject><subject>Biological and Medical Physics</subject><subject>Biophysics</subject><subject>Fields</subject><subject>Molecular</subject><subject>Nuclei</subject><subject>Optical and Plasma Physics</subject><subject>Particle and Nuclear Physics</subject><subject>Particles</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Information Technology</subject><subject>Solid State Physics</subject><subject>Spintronics</subject><issn>0021-3640</issn><issn>1090-6487</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNp9kM1OwzAQhC0EEqXwANz8AoFdx_XPEVX8iQIH4Bw5yYamau3ITkV5exIKJyROq9XMt9oZxs4RLhBzefkCIDBXEnCGAKDsAZsgWMiUNPqQTUY5G_VjdpLSCgDR5HrCuif64LTrKLYb8j0PnidysVryJkTeL4lHSsE7XxF3ZQqx69vBExqewtpF7nbjSpu276nmrf9GHpH30fnU_npN_hC531Zrak_ZUePWic5-5pS93Vy_zu-yxfPt_fxqkVVorc1KqE2Vg6uF1qUzhlyjNGmyppaVAJClEiCkUkYLtFI4C6WcSQG6wVkp6nzKcH-3iiGlSE3RDRFd_CwQirGy4k9lAyP2TBq8_p1isQrb6Ic3_4G-APVnbSI</recordid><startdate>201505</startdate><enddate>201505</enddate><creator>Gavrilyuk, Yu. M.</creator><creator>Gangapshev, A. N.</creator><creator>Derbin, A. V.</creator><creator>Drachnev, I. S.</creator><creator>Kazalov, V. V.</creator><creator>Kobychev, V. V.</creator><creator>Kuz’minov, V. V.</creator><creator>Muratova, V. N.</creator><creator>Panasenko, S. I.</creator><creator>Ratkevich, S. S.</creator><creator>Semenov, D. A.</creator><creator>Tekueva, D. A.</creator><creator>Unzhakov, E. V.</creator><creator>Yakimenko, S. P.</creator><general>Pleiades Publishing</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>201505</creationdate><title>New experiment on search for the resonance absorption of solar axion emitted in the M1 transition of 83Kr nuclei</title><author>Gavrilyuk, Yu. M. ; Gangapshev, A. N. ; Derbin, A. V. ; Drachnev, I. S. ; Kazalov, V. V. ; Kobychev, V. V. ; Kuz’minov, V. V. ; Muratova, V. N. ; Panasenko, S. I. ; Ratkevich, S. S. ; Semenov, D. A. ; Tekueva, D. A. ; Unzhakov, E. V. ; Yakimenko, S. P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1999-b0d8c30ad277ba88eaf67e7e98d4c2004b62024668721942a90b454207f15b2d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Atomic</topic><topic>Biological and Medical Physics</topic><topic>Biophysics</topic><topic>Fields</topic><topic>Molecular</topic><topic>Nuclei</topic><topic>Optical and Plasma Physics</topic><topic>Particle and Nuclear Physics</topic><topic>Particles</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Information Technology</topic><topic>Solid State Physics</topic><topic>Spintronics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gavrilyuk, Yu. M.</creatorcontrib><creatorcontrib>Gangapshev, A. N.</creatorcontrib><creatorcontrib>Derbin, A. V.</creatorcontrib><creatorcontrib>Drachnev, I. S.</creatorcontrib><creatorcontrib>Kazalov, V. V.</creatorcontrib><creatorcontrib>Kobychev, V. V.</creatorcontrib><creatorcontrib>Kuz’minov, V. V.</creatorcontrib><creatorcontrib>Muratova, V. N.</creatorcontrib><creatorcontrib>Panasenko, S. I.</creatorcontrib><creatorcontrib>Ratkevich, S. S.</creatorcontrib><creatorcontrib>Semenov, D. A.</creatorcontrib><creatorcontrib>Tekueva, D. A.</creatorcontrib><creatorcontrib>Unzhakov, E. V.</creatorcontrib><creatorcontrib>Yakimenko, S. P.</creatorcontrib><collection>CrossRef</collection><jtitle>JETP letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gavrilyuk, Yu. M.</au><au>Gangapshev, A. N.</au><au>Derbin, A. V.</au><au>Drachnev, I. S.</au><au>Kazalov, V. V.</au><au>Kobychev, V. V.</au><au>Kuz’minov, V. V.</au><au>Muratova, V. N.</au><au>Panasenko, S. I.</au><au>Ratkevich, S. S.</au><au>Semenov, D. A.</au><au>Tekueva, D. A.</au><au>Unzhakov, E. V.</au><au>Yakimenko, S. P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>New experiment on search for the resonance absorption of solar axion emitted in the M1 transition of 83Kr nuclei</atitle><jtitle>JETP letters</jtitle><stitle>Jetp Lett</stitle><date>2015-05</date><risdate>2015</risdate><volume>101</volume><issue>10</issue><spage>664</spage><epage>669</epage><pages>664-669</pages><issn>0021-3640</issn><eissn>1090-6487</eissn><abstract>Axions with an energy of 9.4 keV emitted in the
M
1 transition of
83
Kr nuclei in the Sun have been sought in the resonance absorption reaction
A
+
83
Kr →
83
Kr* →
83
Kr + γ,
e
(9.4 keV). A proportional gas chamber filled with krypton and placed in a low-background setup at the underground laboratory of the Baksan neutrino observatory was used to detect γ-ray photons and electrons appearing after the decay of a nuclear level. As a result, a new constraint has been determined on the isoscalar and isovector coupling constants of the axion with nucleons: |
g
AN
3
–
g
AN
0
| ≤ 1.29 × 10
–6
. This constraint results in the following new bound on the mass of the axion in the hadronic axion model:
m
A
≤ 100 eV (95% C.L.).</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0021364015100069</doi><tpages>6</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0021-3640 |
| ispartof | JETP letters, 2015-05, Vol.101 (10), p.664-669 |
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| subjects | Atomic Biological and Medical Physics Biophysics Fields Molecular Nuclei Optical and Plasma Physics Particle and Nuclear Physics Particles Physics Physics and Astronomy Quantum Information Technology Solid State Physics Spintronics |
| title | New experiment on search for the resonance absorption of solar axion emitted in the M1 transition of 83Kr nuclei |
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