Thursday, December 03, 2020
9:00 AM -
9:55 AM
Online Event
Analysis Seminar
Series: Analysis Seminar Series
Dynamics of Newtonian stars
A classical model to describe the dynamics of Newtonian stars is the gravitational Euler-Poisson system. The Euler-Poisson system admits a wide range of star solutions that are in equilibrium or expand for all time or collapse in a finite time or rotate. In this talk, I will discuss some recent progress on those star solutions with focus on expansion and collapse
Event Sponsors:
For more information, please contact Math Department by phone at 626-395-4335 or by email at [email protected].