邀请人 (Invited by): 李刚

时间 (Time): 星期一，2023/04/3-15：00-16：00

地点 (Location): 珠海校区天琴中心2316会议室

摘要 (Abstract): 

Future studies of dark matter (DM) will be interdisciplinary, which include cosmological and astrophysical constraints, indirect signals and direct detections. A synergy study of DM consistently with all those channels is the key to robust physics of DM. By overviewing the evidence for the DM hypothesis, I first discuss some cosmological and astrophysical probes for “model independent” DM properties, such as the “coldness” and interactions. The often-considered DM candidates, e.g., WIMP and ALP, are in tension with observations, which motivates new proposals for DM. I will talk about a recently proposed B-L gauge. The model consistent with cosmological constraints predicts a nontrivial neutrino signal potentially detectable in the future with low-energy neutrino experiments. In addition, remarks will be given on several cosmological anomalies and their DM explanation. In the future, small-scale dwarf systems and the cosmic dawn are promising for DM properties searches due to their less contaminations.

主讲人简介 (Speaker's CV): 

林伟康博士，现为上海交通大学李政道研究所博士后；2018年8月，获得美国德克萨斯大学达拉斯分校宇宙学博士学位；2018年9月至2020年10月，为北卡莱罗纳州立大学博士后。他的主要研究兴趣是宇宙学，但是对跨学科的研究非常感兴趣。他最近的研究包括哈勃常数疑难、暗能量和暗物质，以及量化观测结果不一致性的方法。