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Hunting for dark matter with ultra-stable fibre as frequency delay system

机译:用超稳定纤维作为频率延迟系统狩猎暗物质

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摘要

Many cosmological observations point towards the existence of dark-matter(DM) particles and consider them as the main component of the matter content of the universe. The goal of revealing the nature of dark-matter has triggered the development of new, extremely sensitive detectors. It has been demonstrated that the frequencies and phases of optical clock have a transient shift during the DMs’ arrival due to the DM-SM(Standard Model) coupling. A simple, reliable and feasible experimental scheme is firstly proposed in this paper, based on “frequency-delay system” to search dark-matter by “self-frequency comparison” of an optical clock. During the arrival of a dark-matter, frequency discrepancy is expected between two signals with a short time difference(~ ms ) of the same optical clock to exhibit the interaction between atoms and dark-matter. Furthermore, this process can determine the exact position of dark-matter when it is crossing the optical clocks, therefore a network of detecting stations located in different places is recommended to reduce the misjudgment risk to an acceptable level.
机译:许多宇宙学观察指向暗物质(DM)颗粒的存在,并认为它们是宇宙物质含量的主要成分。揭示暗物质本质的目标引发了新的极其敏感的探测器的发展。已经证明,由于DM-SM(标准模型)耦合,光学时钟的频率和阶段具有在DMS到达期间的瞬态移位。本文首先基于“频率延迟系统”,通过光学时钟的“自频比较”来搜索暗物质的简单,可靠和可行的实验方案。在黑暗物质到达期间,在具有相同光学时钟的短时间差(〜MS)的两个信号之间预期频率差异,以表现出原子和暗物质之间的相互作用。此外,该过程可以在交叉光学时钟时确定暗物质的确切位置,因此建议在不同位置的检测站网络以降低可接受的水平的误判风险。

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