Detectable electric current induced by the dark matter axion in a conductor

被引:3
作者
Iwazaki, Aiichi [1 ]
机构
[1] Nishogakusha Univ, Int Econ & Polit, Chiyoda Ku, 6-16 3 Bantyo, Tokyo 1028336, Japan
关键词
INVARIANCE;
D O I
10.1093/ptep/ptab170
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We propose a method of detecting the dark matter axion by using two slabs of a conductor. The flat surfaces are set face to face, parallel to each other. An external magnetic field B parallel to the surfaces is applied. Radiation converted from the axion arises between the two slabs. When we tune the spacing l between the two surfaces such that l = pi/m(a) with axion mass m(a), a resonance occurs so that the radiation becomes strong. Furthermore, the electric current flowing on the surface of the slabs is enhanced. We show that the electric current is large enough to be detectable at the resonance. It reaches 0.7 x 10(-9) A (10(-5) eV/m(a))(1/2) (B/5 T) (L/10 cm) (sigma/3.3 x 10(7) eV) using 6N copper for the square slabs with side length L and high electrical conductivity sigma at temperature T similar to 1 K. The power of the Joule heating is 0.3 x 10(-22) W (B/5T)(2) (10(-5) eV/m(a))(1/2) (L/10 cm)(2) (sigma/3.3 x 10(7) eV). When we amplify the power using an LC circuit with factor Q(LC), the signal-to-noise ratio is 4.5 x 10(4) (Q(LC)/10(6))(B/5T)(2) (t(obs)/1 s)(1/2) (10(-5) eV/m(a))(L/10 cm)(2) (sigma/3.3 x 10(7) eV) with an observation time of t(obs).
引用
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页数:10
相关论文
共 25 条
[1]   A COSMOLOGICAL BOUND ON THE INVISIBLE AXION [J].
ABBOTT, LF ;
SIKIVIE, P .
PHYSICS LETTERS B, 1983, 120 (1-3) :133-136
[2]  
Anastassopoulos V, 2017, NAT PHYS, V13, P584, DOI [10.1038/NPHYS4109, 10.1038/nphys4109]
[3]   Extended Search for the Invisible Axion with the Axion Dark Matter Experiment [J].
Braine, T. ;
Cervantes, R. ;
Crisosto, N. ;
Du, N. ;
Kimes, S. ;
Rosenberg, L. J. ;
Rybka, G. ;
Yang, J. ;
Bowring, D. ;
Chou, A. S. ;
Khatiwada, R. ;
Sonnenschein, A. ;
Wester, W. ;
Carosi, G. ;
Woollett, N. ;
Duffy, L. D. ;
Bradley, R. ;
Boutan, C. ;
Jones, M. ;
LaRoque, B. H. ;
Oblath, N. S. ;
Taubman, M. S. ;
Clarke, J. ;
Dove, A. ;
Eddins, A. ;
O'Kelley, S. R. ;
Nawaz, S. ;
Siddiqi, I ;
Stevenson, N. ;
Agrawal, A. ;
Dixit, A., V ;
Gleason, J. R. ;
Jois, S. ;
Sikivie, P. ;
Solomon, J. A. ;
Sullivan, N. S. ;
Tanner, D. B. ;
Lentz, E. ;
Daw, E. J. ;
Buckley, J. H. ;
Harrington, P. M. ;
Henriksen, E. A. ;
Murch, K. W. .
PHYSICAL REVIEW LETTERS, 2020, 124 (10)
[4]   THE NOT-SO-HARMLESS AXION [J].
DINE, M ;
FISCHLER, W .
PHYSICS LETTERS B, 1983, 120 (1-3) :137-141
[5]   A SIMPLE SOLUTION TO THE STRONG CP PROBLEM WITH A HARMLESS AXION [J].
DINE, M ;
FISCHLER, W ;
SREDNICKI, M .
PHYSICS LETTERS B, 1981, 104 (03) :199-202
[6]   Searching for WISPy cold dark matter with a dish antenna [J].
Horns, Dieter ;
Jaeckel, Joerg ;
Lindner, Axel ;
Lobanov, Andrei ;
Redondo, Javier ;
Ringwald, Andreas .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2013, (04)
[7]  
Iwazaki A., ARXIV211102564HEPPH
[8]  
Iwazaki A., ARXIV210706514HEPPH
[9]   Axion-radiation conversion by super and normal conductors [J].
Iwazaki, Aiichi .
NUCLEAR PHYSICS B, 2021, 963
[10]   A new method for detecting axion with cylindrical superconductor [J].
Iwazaki, Aiichi .
PHYSICS LETTERS B, 2020, 811