Seminar:- High-energy Astrophysics of the Sun: Problems and Prospects
The Sun is a high-energy astrophysical source due to secondary emissions from cosmic-ray interactions in the solar atmosphere. However, recent observations showed that the observed gamma-ray emission is much higher than previously expected. The speaker will talk about the latest observational results, our current understandings on how the cosmic-ray interactions occur, prospects for future detectors, and lastly, the implication of these studies on dark matter searches from the Sun.
時間:2016.04.15(五) 16:30
地點:香港大學 莊月明物理樓 522室
講者:Mr Kenny Chun-Yu Ng 吳震宇 (The Ohio State University)
語言:英語
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【訊息由張詠倫提供】
此活動由香港大學物理學系主辦。