Axion searches in the past, at present, and in the near future

被引:42
作者
Battesti, Remy [1 ]
Beltran, Berta [2 ]
Davoudiasl, Hooman [3 ]
Kuster, Markus [4 ,5 ]
Pugnat, Pierre [6 ]
Rabadan, Raoul [7 ]
Ringwald, Andreas [8 ]
Spooner, Neil [9 ]
Zioutas, Konstantin [10 ]
机构
[1] CNRS, INSA, UPS, Lab Natl champs Magnet Pulses, F-31400 Toulouse, France
[2] Univ Alberta, Dept Phys, Edmonton 1132289, AB, Canada
[3] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[4] Tech Univ Darmstadt, IKP, Petersenstr 30, D-64289 Darmstadt, Germany
[5] Max Planck Inst Extraterr Phys, Karl Schwarzschild Str 1, D-85748 Garching, Germany
[6] European Org Nucl Res CERN, CH-1211 Geneva, Switzerland
[7] Inst Adv Study, Princeton, NJ 08540 USA
[8] Deutsches Elektronen Synchrotron DESY, D-22607 Hamburg, Germany
[9] Univ Sheffield, Sheffield S3 7RH, S Yorkshire, England
[10] Univ Patras, Patras 26500, Greece
来源
AXIONS: THEORY, COSMOLOGY, AND EXPERIMENTAL SEARCHES | 2008年 / 741卷
关键词
D O I
10.1007/978-3-540-73518-2-10
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Theoretical axion models state that axions are very weakly-interacting particles. In order to experimentally detect them, the use of colorful and inspired techniques become mandatory. There are a wide variety of experimental approaches that were developed during the last 30 years; most of them make use of the Primakoff effect, by which axions convert into photons in the presence of an electromagnetic field. We review the experimental techniques used to search for axions and will give an outlook on experiments planned for the near future.
引用
收藏
页码:199 / +
页数:5
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