New indirect search for dark matter

by Prof. Fapeng Huang (TianQin center, Sun Yat-Sen University)

Tuesday 30 Mar 2021, 10:00 → 11:00 Asia/Shanghai

Tsung-Dao Lee library/Fourth Floor-410 - 410# Meeting Room (Tsung-Dao Lee Library)

Abstract:

Motivated by the absence WIMP dark matter signals at LHC and dark matter direct search,we study new indirect search for dark matter by radio signals and gravitational waves signals. For very light dark matter, they can resonantly converted into radio signals in the solar corona or the magnetosphere of neutron star, and then be detected by SKA/FAST.For heavy dark matter, they could be produced during a strong first-order phase transition in the early universe or trigger a strong first-order phase transition. 

Gravitational wave signal could be used to probe these types of dark matter.

Biography:

2010.09-2015.07 Ph.D in Peking University;
2015.06-2017.08 Postdoctor in IHEP;
2017.09-2019.08 Research fellow at IBS-CTPU, South Korea;
2019.09-2021.02 Postdoctoral research associate at Washington university in St.Louis;
From 2021.02 Associate professor at TianQin center, Sun Yat-Sen University.

Meeting room:  https://zoom.com.cn/j/93579891950 

Password:  123456

黄发朋暗物质.pdf