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首页> 外文期刊>Bulletin of the American Physical Society >APS -2017 Annual Meeting of the APS Mid-Atlantic Section- Event - Measuring Gravitational Lensing of the Cosmic Microwave Background to Probe the Mass of the Neutrinos and the Properties of Dark Matter
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APS -2017 Annual Meeting of the APS Mid-Atlantic Section- Event - Measuring Gravitational Lensing of the Cosmic Microwave Background to Probe the Mass of the Neutrinos and the Properties of Dark Matter

机译:APS -2017年APS大西洋中部分会年会-事件-测量宇宙微波背景的引力透镜以探测中微子的质量和暗物质的性质

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In this talk I will discuss the next frontier of research on the Cosmic Microwave Background (CMB): precisely measuring the gravitational lensing of the CMB. This CMB lensing signal encodes a wealth of statistical information about the distribution of matter in the Universe, which is sensitive to the total mass of the neutrinos and the particle properties of dark matter. I will discuss recent progress in probing the sum of the neutrino masses using data from the Atacama Cosmology Telescope Polarimeter (ACTPol), and forecasts of what can be expected from the near future AdvACT, Simons Observatory, and CMB-S4 experiments. I will also discuss a novel and powerful way to probe dark matter particle properties using very high resolution CMB lensing measurements, which can distinguish between cold dark matter and alternative dark matter models that suppress small-scale structure, such as warm or fuzzy dark matter.
机译:在本演讲中,我将讨论宇宙微波背景(CMB)研究的下一个前沿领域:精确测量CMB的引力透镜。该CMB透镜信号编码了有关宇宙中物质分布的大量统计信息,该信息对中微子的总质量和暗物质的粒子特性敏感。我将讨论使用来自阿塔卡马宇宙望远镜偏振计(ACTPol)的数据探测中微子总和的最新进展,以及对不久的AdvACT,西蒙斯天文台和CMB-S4实验的预期结果。我还将讨论使用超高分辨率CMB透镜测量来探测暗物质粒子特性的新颖而有效的方法,该方法可以区分冷暗物质和抑制小规模结构(例如温暖或模糊暗物质)的替代暗物质模型。

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