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Calibrating Ia Supernova Absolute Luminosities using the Distance-Duality Relation
Hunting for Cosmic Baryons
WISE-selected, hyperluminous dust-obscured galaxies: IR SED decomposition and host galaxy morphology
爱因斯坦探针:时域天文发现的机遇
Loop quantum cosmology and alternatives to inflation
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Recent Work on Galactic Dynamics
Superconducting Detectors for Millimeter/Submillimeter Astronomy
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    High Energy Neutrino Astronomy

     

    报告人:Prof. Zhuo Li (KIAA)

     

    时间:2016年5月11日下午4:00

    地点:东区理化大楼18层天文台报告厅

     

    报告摘要: IceCube at the south pole had reported the discovery of TeV-PeV extraterrestrial neutrinos, which open a brand new window to observe the universe. I will briefly overview the history of the high energy neutrino detection, and then discuss the possible origins of these high energy neutrinos. I will emphasize that the multi-messenger approach may be the best way to diagnose the neutrino origin. By the photon-neutrino connection in the neutrino production processes, we can use the Fermi-LAT observations of various objects to constrain their neutrino flux, and test if they could be the sources of the IceCube detected neutrinos.


     
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