报告题目：
Title: The mathematical modelling of white dwarfs, neutron stars and black holes.
（白矮星、中子星和黑洞的数学建模）
报告人: Lilia Ferrario 教授
报告时间：2017年05月04日 10:20-12:00
报告地点：闻天楼 西报告厅
主讲人简介：Lilia Ferrario 教授
职位：Associate Director Education, Mathematical Sciences Institute
澳大利亚国立大学数学科学研究院 分管教育副院长
学历：PhD, The Australian National University 澳大利亚国立大学 博士
研究领域：Stellar Astronomy And Planetary Systems 恒星天文学及行星系统;020110 Mathematical Aspects Of General Relativity 广义相对论的数学方面;010504 Numerical And Computational Mathematics 数学与计算数学；Astronomical And Space Sciences 天文和空间科学
报告内容介绍：
The talk comprises the origin of compact stars, those extremely dense, dead remains of stars that no longer burn nuclear fuel in their interior and the mathematical prediction of black holes. Also discussed will be the exotic properties of the highly magnetic white dwarfs, the rapidly spinning pulsars, and the mysterious 'magnetars.’ Finally, Prof Ferrario will introduce the topic of magnetic accretion and its mathematical modelling. She will show how strongly magnetic compact stars slowly devour their companions and produce the most spectacular phenomena observed in the universe.
本讲座内容包括致密星的起源，内部核燃料停止燃烧的密集死亡恒星和黑洞的数学预测的起源，还将讨论高磁性白矮星的特性，快速旋转的脉冲星和神秘的“磁星”。最后，Ferrario教授将介绍磁性吸积及其数学建模。她将展示致密星是如何通过强磁性慢慢吞噬同伴，并制造了宇宙中最壮观的现象。
