论文标题
起伏的暗物质
Undulating Dark Matter
论文作者
论文摘要
我们建议,显微镜和宏观物理学之间的相互作用会引起暗物质(DM),这些暗物质与可见的部门的相互作用从根本上起伏,而与天体动力学无关。 Fermionic DM提供了一个具体的示例,该示例由振荡的轴突状场产生,导致散射速率下降。可以通过搜索起伏的散射速率来增强光DM搜索的发现潜力,尤其是在背景速率较大且难以估计的检测区域,例如1 MEV附近的DM质量,其中DM电子散射主要在单个电子箱中占主导地位。发现后,起伏的信号还可以揭示宝贵的黑暗扇区信息。在这方面,我们强调的是,如果最近的Xenon1t事件过量是由于光放热的光散射引起的,那么对事件的时间依赖性的未来分析可能会为推定信号的显微镜起源提供线索。
We suggest that an interplay between microscopic and macroscopic physics can give rise to dark matter (DM) whose interactions with the visible sector fundamentally undulate in time, independent of celestial dynamics. A concrete example is provided by fermionic DM with an electric dipole moment (EDM) sourced by an oscillating axion-like field, resulting in undulations in the scattering rate. The discovery potential of light DM searches can be enhanced by additionally searching for undulating scattering rates, especially in detection regions where background rates are large and difficult to estimate, such as for DM masses in the vicinity of 1 MeV where DM-electron scattering dominantly populates the single electron bin. An undulating signal could also reveal precious dark sector information after discovery. In this regard we emphasise that, if the recent XENON1T excess of events is due to light DM scattering exothermically off electrons, future analyses of the time-dependence of events could offer clues as to the microscopic origins of the putative signal.