New generation low-energy probes for ultralight axion and scalar dark matter

被引:10
作者
Stadnik, Yevgeny V. [1 ]
Flambaum, Victor V. [1 ,2 ]
机构
[1] Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia
[2] Johannes Gutenberg Univ Mainz, Mainz Inst Theoret Phys, D-55122 Mainz, Germany
基金
澳大利亚研究理事会;
关键词
Dark matter; axion; scalar; strong CP problem; classical field; topological defect; MAGNETIC MONOPOLES; CP CONSERVATION; COSMIC STRINGS; DOMAIN-WALLS; SOLAR AXIONS; CONSTRAINTS; INVARIANCE; PARTICLES; CONSTANTS; COUPLINGS;
D O I
10.1142/S0217732317400041
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a brief overview of a new generation of high-precision laboratory and astro-physical measurements to search for ultralight (sub-eV) axion, axion-like pseudoscalar and scalar dark matter (DM), which form either a coherently oscillating classical field or topological defects (solitons). In these new detection methods, the sought effects are linear in the interaction constant between DM and ordinary matter, which is in stark contrast to traditional searches for DM, where the sought effects are quadratic or higher order in the underlying interaction constants (which are extremely small).
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页数:12
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