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Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm. / Derbin, A. V.; Bakhlanov, S. B.; Egorov, A. I.; Mitropolsky, I. A.; Muratova, V. N.; Semenov, D. A.; Unzhakov, E. V.

в: Bulletin of the Russian Academy of Sciences: Physics, Том 74, № 4, 01.04.2010, стр. 481-486.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Derbin, AV, Bakhlanov, SB, Egorov, AI, Mitropolsky, IA, Muratova, VN, Semenov, DA & Unzhakov, EV 2010, 'Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm', Bulletin of the Russian Academy of Sciences: Physics, Том. 74, № 4, стр. 481-486. https://doi.org/10.3103/S106287381004012X

APA

Derbin, A. V., Bakhlanov, S. B., Egorov, A. I., Mitropolsky, I. A., Muratova, V. N., Semenov, D. A., & Unzhakov, E. V. (2010). Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm. Bulletin of the Russian Academy of Sciences: Physics, 74(4), 481-486. https://doi.org/10.3103/S106287381004012X

Vancouver

Derbin AV, Bakhlanov SB, Egorov AI, Mitropolsky IA, Muratova VN, Semenov DA и пр. Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm. Bulletin of the Russian Academy of Sciences: Physics. 2010 Апр. 1;74(4):481-486. https://doi.org/10.3103/S106287381004012X

Author

Derbin, A. V. ; Bakhlanov, S. B. ; Egorov, A. I. ; Mitropolsky, I. A. ; Muratova, V. N. ; Semenov, D. A. ; Unzhakov, E. V. / Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm. в: Bulletin of the Russian Academy of Sciences: Physics. 2010 ; Том 74, № 4. стр. 481-486.

BibTeX

@article{1ff0870ae64e4362a6e34afd7e02b8be,
title = "Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm",
abstract = "We searched for resonant excitation of the first excited state of the 169Tm nucleus by axions formed inside the Sun by the Primakoff effect, A + 169Tm → 169Tm* → 169Tm + γ (8.41keV). Gamma quanta with an energy of 8.41keV were registered by a sectionalized Si(Li) detector installed in a low-background setup. As a result, we set a new upper limit for the photon to axion coupling constant, gAγ(GeV-1)mA(eV) ≤ 1.06 × 10-5, which for a hadronic axion model corresponds to a mass limit of mA ≤ 169 eV at a 90% confidence level.",
author = "Derbin, {A. V.} and Bakhlanov, {S. B.} and Egorov, {A. I.} and Mitropolsky, {I. A.} and Muratova, {V. N.} and Semenov, {D. A.} and Unzhakov, {E. V.}",
year = "2010",
month = apr,
day = "1",
doi = "10.3103/S106287381004012X",
language = "English",
volume = "74",
pages = "481--486",
journal = "Bulletin of the Russian Academy of Sciences: Physics",
issn = "1062-8738",
publisher = "Allerton Press, Inc.",
number = "4",

}

RIS

TY - JOUR

T1 - Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm

AU - Derbin, A. V.

AU - Bakhlanov, S. B.

AU - Egorov, A. I.

AU - Mitropolsky, I. A.

AU - Muratova, V. N.

AU - Semenov, D. A.

AU - Unzhakov, E. V.

PY - 2010/4/1

Y1 - 2010/4/1

N2 - We searched for resonant excitation of the first excited state of the 169Tm nucleus by axions formed inside the Sun by the Primakoff effect, A + 169Tm → 169Tm* → 169Tm + γ (8.41keV). Gamma quanta with an energy of 8.41keV were registered by a sectionalized Si(Li) detector installed in a low-background setup. As a result, we set a new upper limit for the photon to axion coupling constant, gAγ(GeV-1)mA(eV) ≤ 1.06 × 10-5, which for a hadronic axion model corresponds to a mass limit of mA ≤ 169 eV at a 90% confidence level.

AB - We searched for resonant excitation of the first excited state of the 169Tm nucleus by axions formed inside the Sun by the Primakoff effect, A + 169Tm → 169Tm* → 169Tm + γ (8.41keV). Gamma quanta with an energy of 8.41keV were registered by a sectionalized Si(Li) detector installed in a low-background setup. As a result, we set a new upper limit for the photon to axion coupling constant, gAγ(GeV-1)mA(eV) ≤ 1.06 × 10-5, which for a hadronic axion model corresponds to a mass limit of mA ≤ 169 eV at a 90% confidence level.

UR - http://www.scopus.com/inward/record.url?scp=77953355675&partnerID=8YFLogxK

U2 - 10.3103/S106287381004012X

DO - 10.3103/S106287381004012X

M3 - Article

AN - SCOPUS:77953355675

VL - 74

SP - 481

EP - 486

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

SN - 1062-8738

IS - 4

ER -

ID: 42278390