uc-berkeley-00-rixin-li.md

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/team/rixin-li/	Li, Rixin	University of California, Berkeley	51 Pegasi b Postdoctoral Fellow	teaser /assets/images/team/rixin-li.png	title image text Position /assets/images/team/rixin-li.png 51 Pegasi b Postdoctoral Fellow<br> <a href='https://ui.adsabs.harvard.edu/search/q=orcid%3A0000-0001-9222-4367&sort=date%20desc%2C%20bibcode%20desc&p_=0' target='_blank'><i class='fas fa-fw fa-search'></i>ADS</a><br> <a href='https://scholar.google.com/citations?user=cEJjBwIAAAAJ&hl=en' target='_blank'><i class='fas fa-fw fa-user-graduate'></i>Google Scholar</a><br> <a href='mailto:rixin@berkeley.edu'><i class='fas fa-fw fa-envelope'></i>Email</a><br> title text Research Interests <ul> <li> Planet Formation <li> [Dusty] Accretion Disks <li> Gravitational Wave Sources <li> Computational / Theoretical Astrophysics

Rixin Li (李日新) is a 51 Pegasi b Postdoctoral Fellow in the Department of Astronomy at the University of California, Berkeley. His research uses numerical simulations to understand the evolution of dusty circumstellar disks, the formation of planets therein, and the astrophysics of black holes in AGN disks, from which he makes observable predictions to test the underlying theories.

Biography

• 2023–present - 51 Pegasi b Postdoctoral Fellow, University of California, Berkeley
• 2020–2023 - Postdoctoral Research Associate, Cornell University
• 2014-2020 - Ph.D., University of Arizona
• 2010-2014 - B.Sc., Peking University