报告摘要：The Chinese Space Station Telescope (CSST) and other international surveys make it fitting to reconsider previously ignored relativistic effects in the dynamics of galaxies. Here I will show how such effects allow observers to measure directly the gravitational potentials and proper motions of galaxies and clusters, and argue why these new and direct measurements could be routinely made with future large instruments.
个人简介：赵红胜是暗晕引力领域资深教授、皇家天 文协会会士、多期刊编辑、暗晕赵模型 (Zhao Profile)的提出者，在宏观暗晕引力势重构、微观暗粒子探测、引力论扩展三 大方向发表含天文/物理通讯的第一作者 论文50篇，获海外青年基金、剑桥科维里、法国古腾堡、荷兰自然科学等基金资 助和BBC、科学美国人等多国媒体采访， 培养的人才获德国洪堡、海外正高职位及 中科院百人计划等。