Tunable Axion Plasma Haloscopes

被引:152
|
作者
Lawson, Matthew [1 ,2 ,3 ]
Millar, Alexander J. [1 ,2 ,3 ]
Pancaldi, Matteo [4 ]
Vitagliano, Edoardo [5 ]
Wilczek, Frank [1 ,2 ,3 ,6 ,7 ,8 ,9 ]
机构
[1] Stockholm Univ, Dept Phys, AlbaNova, Oskar Klein Ctr Cosmoparticle Phys, S-10691 Stockholm, Sweden
[2] KTH Royal Inst Technol, NORDITA, Roslagstullsbacken 23, S-10691 Stockholm, Sweden
[3] Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden
[4] Stockholm Univ, Dept Phys, AlbaNova, S-10691 Stockholm, Sweden
[5] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Fohringer Ring 6, D-80805 Munich, Germany
[6] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA
[7] TD Lee Inst, Shanghai 200240, Peoples R China
[8] Shanghai Jiao Tong Univ, Dept Phys & Astron, Wilczek Quantum Ctr, Shanghai 200240, Peoples R China
[9] Arizona State Univ, Dept Phys & Origins Project, Tempe, AZ 25287 USA
基金
欧盟地平线“2020”; 瑞典研究理事会; 欧洲研究理事会;
关键词
LIGHT; CAVITY; SEARCH;
D O I
10.1103/PhysRevLett.123.141802
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We propose a new strategy for searching for dark matter axions using tunable cryogenic plasmas. Unlike current experiments, which repair the mismatch between axion and photon masses by breaking translational invariance (cavity and dielectric haloscopes), a plasma haloscope enables resonant conversion by matching the axion mass to a plasma frequency. A key advantage is that the plasma frequency is unrelated to the physical size of the device, allowing large conversion volumes. We identify wire metamaterials as a promising candidate plasma, wherein the plasma frequency can be tuned by varying the interwire spacing. For realistic experimental sizes, we estimate competitive sensitivity for axion masses of 35-400 mu eV, at least.
引用
收藏
页数:7
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