Abstract:
Stars communicate with us via signals carried by disparate "messengers", including electromagnetic radiation, gravitational waves, neutrinos, and cosmic rays. The accurate determination of crucial nuclear reaction rates is paramount in deciphering these encoded messages, thereby revealing the hidden truths within stars and ultimately shedding light on the origins of elements. In this presentation, I will elucidate how nuclear astrophysicists synthesize elements using laboratory accelerators and study stellar nucleosynthetic processes through a review of some important experiments conducted by our group, such as the Jinping Underground Nuclear Astrophysics (JUNA) experiment, the direct measurement of the 12C+12C reaction rate, and the stellar lifetime of 59Fe. My perspectives on experimental nuclear astrophysics will also be presented.
Biography:
Professor Tang is an expert in nuclear astrophysics. He is currently a principal scientist of nuclear astrophysics at the Institute of Modern Physics (IMP), CAS, and an adjunct professor of Lanzhou University. He completed his physics undergraduate studies at Nanjing University, master studies at China Institute of Atomic Energy, and his Ph.D. in nuclear physics at Texas A&M University. Before he joined IMP, he was a postdoc at Argonne National Laboratory and also was an assistant professor of physics at the University of Notre Dame. He is a member of CPS, APS, SPS, and OCPA.
Host: Prof. Jianglai Liu
Alternative online link: https://meeting.tencent.com/dm/hbXkzwh7AMAm (id: 468886610 passcode: 123456)