Looking for dark sector

by Dr Xiaoping Wang

Wednesday 20 Mar 2019, 12:00 → 13:00 Asia/Shanghai

数理楼3304 (北京工业大学)

Dark matter contains 85% of the matter density and it is supposed to have a rich structure, same as our complex baryonic world. The dark sector related with the 85% matter density, is defined as particles which do not interact strongly with the Standard Model particles. It contains dark matter as a stable particle, and particles mediating interaction between dark matter and visible sector. We go over the direct, indirect and collider searches for the canonical dark matter candidate, the weakly interacting massive particles. Besides the canonical dark matter candidate, we also study different mass scale dark matter, including PeV dark matter, keV dark matter and fuzzy dark matter, whose mass is only 10^(-22) eV. For the ultralight dark matter phenomenology, we emphasize an interplay with neutrino physics.

 

王小平，美国阿贡国家实验室博士后。主要研究方向粒子物理唯象学，包括暗物质探测，加速器物理和中微子物理。
2014年毕业于北京大学物理系，获理学博士学位。同年进入德国美因茨大学做博士后，2017年到美国阿贡国家实验室做博士后。发表SCI论文22篇，国际大会报告10余次。同时担任prd，cpc，prl等SCI杂志审稿人。