天體物理模型的挑戰 – 宇宙高能量彌散中微子和伽瑪射線背景


Colloquium:- The Cosmic High Energy Diffuse Neutrino and Gamma-ray Backgrounds: Challenges for Astrophysical Models 
 
The IceCube Antarctic Cherenkov telescope has detected a diffuse neutrino background flux at TeV to Pev energies which is of astrophysical origin, while the Fermi spacecraft has detected a diffuse 0.1-300 GeV diffuse gamma-ray background flux, neither of whose origin is obvious. I will discuss several astrophysical source models addressing these issues, including galaxy mergers, star-burst galaxies, low-luminosity gamma-ray bursts and supernovae. 
 
時間:2016.12.06(二) 16:00
地點:香港大學 莊月明物理樓 LG1 P2 演講廳 
講者:Prof. Peter MÉSZÁROS (Pennsylvania 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。

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