Formation Channels of Magnetars
中国科学院云南天文台学术报告通知
2025年第37期
报告题目：Formation Channels of Magnetars
报告人：Ruichong Hu
报告人单位：University of Nevada,Las Vegas
报告时间：2025年8月15日（星期五）10:00-11:30
报告地点：科研1号楼412会议室
报告摘要：
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Magnetars are young neutron stars (NSs) with strong magnetic fields and are associated with various high-energy astrophysical phenomena. In this work, we explore potential magnetar formation channels and quantify their contributions using population synthesis simulations, considering both single-star and isolated binary system evolution. By varying model parameters, we compare the effects of various evolution processes on magnetar formation. Additionally, we study the delay times of magnetar formation across different channels, as well as the properties of magnetars and their companions in binary systems.
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报告人简介：
Ruichong Hu is a Ph.D. student at the University of Nevada,Las Vegas,supervised by Professor Bing Zhang. His research focuses on understanding how different physical processes affect the formation of compact objects (neutron stars and black holes) through numerical simulations of binary evolution.
云台邀请方：大样本恒星演化研究团组、国际超新星中心、云南省国际超新星研究重点实验室
邀请方联系人：陈海亮
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