A Forecast of the Sensitivity of the DALI Experiment to Galactic Axion Dark Matter

被引:4
|
作者
Hernandez-Cabrera, Juan F. [1 ,2 ]
De Miguel, Javier [1 ,2 ,3 ]
Joven alvarez, Enrique [1 ,2 ]
Hernandez-Suarez, E. [1 ,2 ]
Rubino-Martin, J. Alberto [1 ,2 ]
Otani, Chiko [3 ]
机构
[1] Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Tenerife, Spain
[2] Univ La Laguna, Dept Astrofis, E-38206 San Cristobal la Laguna, Tenerife, Spain
[3] Inst Phys & Chem Res RIKEN, Ctr Adv Photon, 519-1399 Aramaki Aoba,Aoba ku, Sendai, Miyagi 9800845, Japan
来源
SYMMETRY-BASEL | 2024年 / 16卷 / 02期
关键词
CP violation; dark matter; Peccei-Quinn symmetry; axion; haloscope; Monte Carlo simulation; INVARIANCE;
D O I
10.3390/sym16020163
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 long-postulated boson that can simultaneously solve two fundamental problems of modern physics: the charge-parity symmetry problem in the strong interaction and the enigma of dark matter. In this work, we estimate, by means of Monte Carlo simulations, the sensitivity of the Dark-photons & Axion-Like particles Interferometer (DALI), a new-generation Fabry-Perot haloscope proposed to probe axion dark matter in the 25-250 mu eV band.
引用
收藏
页数:14
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