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5. Indirect Detection of Dark matter

Indirect Detection of Dark matter

来源 :The Sino-French“LIA-ORIGINS”Workshop in 2014(中法“起源”天文联合实验室20 | 被引量 : 0次 | 上传用户：liongliong536

【摘 要】

：

What Tools Do We Use?Auger and HiRes measure the highest energy cosmic ray flux,spectrum,and anisotropy.ICECube searches for TeV neutrino sources – the most di

【作 者】

：

Bi Xiao-Jun 

【机 构】

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InstituteofHighEnergyPhysics

【出 处】

：

The Sino-French“LIA-ORIGINS”Workshop in 2014(中法“起源”天文联合实验室20

【发表日期】

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2014年10期

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What Tools Do We Use?Auger and HiRes measure the highest energy cosmic ray flux,spectrum,and anisotropy.ICECube searches for TeV neutrino sources – the most direct signature of hadronic acceleratorsFermi detects thousands of new GeV sources.VERITAS,HESS,MAGIC,and CANGAROO image and measure spectra and variability of TeV sources.

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