学术报告（11月13日 周二 14:00 – 15:00）

主 持 人：王为 教授

欢迎广大师生前来参与！

摘要：

In 2013, the IceCube Neutrino Observatory at the geographic South Pole detected a diffuse astrophysical neutrino flux, marking the dawn of high-energy neutrino astronomy. Since then, the campaign of hunting for astrophysical neutrino sources has been on. On September 22, 2017, the IceCube realtime alert system detected a 290 TeV muon neutrino event, which triggered follow-up observations from more than 20 multi-wavelength telescopes around the world. The event was eventually traced back to a flaring blazar TXS0506+056, approximately 4 billion light years away. I will talk about the multi-messenger observation of the blazar neutrino event and its implications.

报告人简介：

2004 – 2008： 中国科学技术大学，天体物理学士

2008 – 2015： University of Alabama-Tuscaloosa, PhD

2015 – 2018：University of Wisconsin – Madison, Postdoc

2018.09 至今：上海交通大学、李政道研究所

主要研究方向：中微子天文学

国际合作组：冰立方(IceCube), 2009年加入。