Axion dark matter: How to see it?

被引:50
|
作者
Semertzidis, Yannis K. [1 ,2 ]
Youn, SungWoo [1 ]
机构
[1] Inst for Basic Sci Korea, Ctr Axion & Precis Phys Res, Daejeon 34051, South Korea
[2] Korea Adv Inst Sci & Technol, Dept Phys, Daejeon 34141, South Korea
关键词
COSMIC AXIONS; SEARCH; INVARIANCE; CONVERSION; PHOTONS; CAVITY;
D O I
10.1126/sciadv.abm9928
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The axion is a highly motivated elementary particle that could address two fundamental questions in physics- the strong charge-parity (CP) problem and the dark matter mystery. Experimental searches for this hypothetical particle started reaching theoretically interesting sensitivity levels, particularly in the micro-electron volt (gigahertz) region. They rely on microwave resonators in strong magnetic fields with signals read out by quantum noise limited amplifiers. Concurrently, there have been intensive experimental efforts to widen the search range by devising various techniques and to enhance sensitivities by implementing advanced technologies. These orthogonal approaches will enable us to explore most of the parameter space for axions and axion-like particles within the next decades, with the 1- to 25-gigahertz frequency range to be conquered well within the first decade. We review the experimental aspects of axion physics and discuss the past, present, and future of the direct search programs.
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页数:13
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