Wave-like Dark Matter and Axions

C. Bartram
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Abstract

Despite composing 85% of the matter in the universe, the exact nature of dark matter is still unknown. The possibility ofwave-like darkmatter and axions is driving a surge of new experiments that are vitalized by progress in quantum amplification and optics, microwave electronics, high magnetic fields, and cryogenics. We discuss the technology that enables such searches, and break down the experiments by their reliance on different axion couplings. We explain how the Axion Dark Matter eXperiment (ADMX) has achieved sensitivity to a particularly compelling class of dark matter candidates, known as DFSZ axions, in a narrow range of axion masses. Finally, with a new fleet of experiments arriving online, we present their goals to probe as yet unexplored parts of axion parameter space in the coming years.
波状暗物质和轴子
尽管构成了宇宙中85%的物质,但暗物质的确切性质仍然未知。波状暗物质和轴子存在的可能性正在推动一大批新实验的兴起,这些实验因量子放大和光学、微波电子学、强磁场和低温学方面的进展而充满活力。我们讨论了实现这种搜索的技术,并通过它们对不同轴子耦合的依赖来分解实验。我们解释了轴子暗物质实验(ADMX)如何在一个狭窄的轴子质量范围内实现对一类特别引人注目的暗物质候选者(称为DFSZ轴子)的敏感性。最后,随着新的实验舰队上线,我们提出了他们在未来几年探索轴子参数空间尚未探索的部分的目标。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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