报告题目: Galaxy Clusters: A Standard Cannon for Cosmology
报告人: Prof.Christopher J Miller(Professor of Astronomy, Professor of Physics, University of Michigan, Ann Arbor USA)
报告摘要:Einstein’s theory of general relativity (GR) entwines the dynamics of matter-energy and the universe's spacetime expansion. Recent authors have revised our understanding of the mathematics of dynamical tracers within the context of GR for an accelerating space-time metric. As a consequence, we have a new understanding of how the escape speed relates to the local potential via the Poisson equation. General relativity requires that the escape velocity for a massive extended object like a galaxy cluster be reduced compared to its Newtonian counterpart. In fact, the combined weak lensing and escape profiles of clusters provide a new dynamical probe of the expansion history of the universe. I will give a description of the theory, results from tests using increasingly realistic simulations, and examples from the first applications of this technique to real data. I will then discuss the future prospects of this new cosmological tool in the context of surveys like LSST and DESI.
报告时间:2023年4月19日(星期三),下午2:00-3:00
报告地点:仙林园区3号楼302会议室
欢迎大家参加!
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