Dielectric haloscopes to search for axion dark matter: theoretical foundations

被引:82
|
作者
Millar, Alexander J. [1 ]
Raffelt, Georg G. [1 ]
Redondo, Javier [1 ,2 ]
Steffen, Frank D. [1 ]
机构
[1] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Fohringer Ring 6, D-80805 Munich, Germany
[2] Univ Zaragoza, P Cerbuna 12, E-50009 Zaragoza, Spain
基金
欧盟地平线“2020”;
关键词
axions; dark matter detectors; dark matter theory; STRONG CP PROBLEM; DOMAIN-WALLS; PHOTON; MODELS;
D O I
10.1088/1475-7516/2017/01/061
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the underlying theory of dielectric haloscopes, a new way to detect dark matter axions. When an interface between different dielectric media is inside a magnetic field, the oscillating axion field acts as a source of electromagnetic waves, which emerge in both directions perpendicular to the surface. The emission rate can be boosted by multiple layers judiciously placed to achieve constructive interference and by a large transverse area. Starting from the axion-modified Maxwell equations, we calculate the efficiency of this new dielectric haloscope approach. This technique could potentially search the unexplored high-frequency range of 10-100 GHz (axion mass 40-400 mu eV), where traditional cavity resonators have difficulties reaching the required volume.
引用
收藏
页数:72
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