Nonlinear stability of non-rotating Newtonian stars.

发布者:王丹丹发布时间:2023-12-11浏览次数:10

江苏省应用数学(中国矿业大学)中心系列学术报告

报告题目:Nonlinear stability of non-rotating Newtonian stars.

报告人:朱昊助理研究员

报告时间:2023/12/12 (周二)15:00-16:00

腾讯会议:5318371238

报告摘要:For the non-rotating gaseous stars modeled by the compressible Euler-Poisson system with general pressure law, Lin and Zeng recently proved a turning point principle, which gives the sharp linear stability/instability criteria for the non-rotating gaseous stars. We prove that the sharp linear stability criterion for the non-rotating stars also conditionally implies nonlinear orbital stability against general perturbations. If the perturbations are further restricted to be spherically symmetric, then nonlinear stability holds true unconditionally.  

报告人简介:朱昊,南京大学数学系助理研究员,博士毕业于山东大学,曾获博新计划资助,主要从事流体动力学和微分算子谱理论等方面的研究。