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高能宇宙线起源的多信使研究

  • 2018年秋季

题目:高能宇宙线起源的多信使研究

报告人:王祥玉 教授 (杰青), 南京大学

时间地点:周四, 2018.11.1下午2:30-4:30, 物理楼552

Abstract:

Cosmic rays are extremely energetic charged particles  with energy up to 10^20 eV. Although these particles have been discovered for more than 100 years, the astrophysical sources of them are still unknown. As cosmic rays produce secondary neutrinos and gamma-rays within the source or during the propagation,  neutrino and gamma-ray are important messengers to study the origin of the parent cosmic rays.  In recent years, a lot of progress has been made in this area, thanks to IceCube and Fermi observatories. I will discuss the multi-messenger approach, incorporating gamma-ray, neutrino and cosmic ray research, in studying the origin of Galactic and extra-Galactic cosmic rays.

简介:王祥玉,1995年本科毕业于南京师范大学物理系,2001年获得南京大学天体物理学博士学位,2005-2007年在美国宾州州立大学从事博士后研究。现为南京大学天文与空间科学学院教授、博士生导师、国家杰出青年基金获得者。主要从事高能宇宙线、伽玛射线暴等天体物理问题的研究。指导的两名研究生获得江苏省优秀博士学位论文奖。




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