Abstract:
Our Milky Way has been observed at different wavelengths, from radio to gamma rays. Until recently, with the breakthroughs in PeV-gamma-ray and TeV-neutrino astronomy brought by the LHAASO and IceCube Collaboration, the sky is getting richer than before. The observations provide fundamental insights into the Galaxy formation, evolutions and intensities and spectra of cosmic rays (CRs). In this talk, based on the updated observations of Galactic diffuse emission, I will present the study of CR properties and the estimation of Galactic neutrino distribution. Furthermore, to map the large-scale emission of our Galaxy with unprecedented precision, the next generation of imaging atmospheric Cherenkov telescopes CTA will be essential, and it will reveal the mystery of dark matter and give answers to open questions in gamma-ray astronomy.
Resume:
Education
2004-2008 B.Sc. Physics, Nankai University
2008-2013 Ph.D. Physics, Arizona State University
Work Experience
2018.9-present Associate Professor, School of Physics and Astronomy, Sun Yat-sen University
2014.9-2018.9 Research Associated/Assistant Professor, Center for Astrophysics and Cosmology, University of Nova Gorica, Slovenia
Scientific Collaborations
2019-present, LHAASO
2019-present, observer, KM3NeT
2014-present, Cherenkov Telescope Array
2014-2018, Pierre Auger Observatory
Online Meeting Room：https://meeting.tencent.com/dm/Gms66QlO48Mm
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