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.

引用

页码：481 / 486

页数：5

共 34 条

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