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

被引：5
|
作者：
Derbin A.V. [1 ]
Bakhlanov S.B. [1 ]
Egorov A.I. [1 ]
Mitropolsky I.A. [1 ]
Muratova V.N. [1 ]
Semenov D.A. [1 ]
Unzhakov E.V. [1 ]
机构：
[1] Konstantinov St. Petersburg Nuclear Physics Institute, Gatchina
来源：
Bulletin of the Russian Academy of Sciences: Physics | 2010年 / 74卷 / 4期
关键词：
Solar Axion; Resonant Absorption; Hadronic Axion; Invisible Axion; Pseudo Scalar Particle;
D O I：
10.3103/S106287381004012X
中图分类号：
学科分类号：
摘要：
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. © Allerton Press, Inc., 2010.
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收藏
页码：481 / 486
页数：5
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