Abstract: In this talk, I'll introduce our recent efforts in modeling the effect of self-interacting dark matter (SIDM) and making contact with small-scale observations. I'll start by reviewing the background of our studies and introducing a parametric model for SIDM halos that enables obtaining theoretical predictions based on a few simple equations. I'll then delve into our dedicated studies addressing various challenges in observations and discuss their implications for SIDM. Confronting the rich and intricate small-scale data, I'll also briefly touch upon our recent endeavors in applying network theory and artificial intelligence in cosmological simulations. I'll comment on the potential prospect of bridging theory and observations through parametrized and graph-inspired models.
请线下参加报告的外单位老师、同学注册时填写个人信息(中文姓名、身份证号码及手机号码),用于预约进入物理学院。
Prof. Q. Li