Abstract
The relativistic protons in the extremely powerful jets of blazars may boost the dark matter (DM) particles in the surrounding of the source to high energy via elastic collision, which opens a new possibility for probing the nature of DM at underground DM direct detection experiments. In this talk, I will focus on two sample sources, i.e. TXS 0506+056 and BL Lacertae, and derive the corresponding limitations of spin-dependent and spin-independent DM-nucleon cross section by using the results of XENON1T, MiniBooNE, and Borexino.
Biography
Education: Scuola Internazionale Superiore di Studi Avanzati (SISSA)
09.2020 – Present Postdoc Collaborator: Prof. Piero Ullio
Department of Physics, University of Pisa
09.2019 – 08.2020 Visiting Ph.D. student (sponsored by the China Scholarship Council)
Collaborator: Prof. Alessandro Strumia
Institute of High Energy Physics, CAS
09.2015 – 07.2020 Ph.D. student in Particle Physics and Nuclear Physics (conferred by the University of Chinese Academy of Sciences)
Supervisor: Prof. Xiao-Jun Bi
Zoom information: https://cern.zoom.us/j/66653186249?pwd=YjFhblJDdzhlbXpBYys2ODlydEJ3Zz09
ID: 666 5318 6249 Password: 856077