Recent Results of Search for Solar Axions Using Resonant Absorption by 83Kr nuclei

被引：2

作者：

Derbin, A. V. ^{[1
]}

Drachnev, I. S. ^{[1
]}

Gangapshev, A. M. ^{[2
]}

Gavrilyuk, Yu M. ^{[2
]}

Kazalov, V. V. ^{[2
]}

Kobychev, V. V. ^{[3
]}

Kuzminov, V. V. ^{[2
]}

Muratova, V. N. ^{[1
]}

Panashenko, S. I. ^{[4
]}

Ratkevich, S. S. ^{[4
]}

Tekueva, D. A. ^{[2
]}

Unzhakov, E. V. ^{[1
]}

Yakimenko, S. P. ^{[2
]}

机构：

[1] NRC Kurchatov Inst, Petersburg Nucl Phys Inst, St Petersburg, Russia

[2] RAS, Inst Nucl Res, Moscow, Russia

[3] NAS Ukraine, Inst Nucl Res, Kiev, Ukraine

[4] Kharkov Natl Univ, Kharkov, Ukraine

来源：

3RD INTERNATIONAL CONFERENCE ON PARTICLE PHYSICS AND ASTROPHYSICS (ICPPA 2017) | 2017年 / 934卷

基金：

俄罗斯科学基金会;

关键词：

M1; TRANSITION;

D O I：

10.1088/1742-6596/934/1/012018

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

A search for resonant absorption of the solar axion by Kr-83 nuclei was performed using the proportional counter installed inside the low-background setup at the Baksan Neutrino Observatory. The obtained model independent upper limit on the combination of isoscalar and isovector axion-nucleon couplings vertical bar g(3) - g(0)vertical bar <= 8.4 x 10(-7) allowed us to set the new upper limit on the hadronic axion mass of m(A) <= 65 eV (95% C.L.) with the generally accepted values S = 0.5 and z = 0.56.

引用

页数：4

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