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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.

In: Bulletin of the Russian Academy of Sciences: Physics, Vol. 74, No. 4, 01.04.2010, p. 481-486.

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

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, vol. 74, no. 4, pp. 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 et al. Search for solar axions generated by the primakoff effect with resonance absorption by 169Tm. Bulletin of the Russian Academy of Sciences: Physics. 2010 Apr 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. In: Bulletin of the Russian Academy of Sciences: Physics. 2010 ; Vol. 74, No. 4. pp. 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