PPT-Arunava Bhadra
Author : phoebe-click | Published Date : 2016-06-24
High Energy amp Cosmic Ray Research Ctr North Bengal University TeV Neutrinos and Gamma rays from PulsarsMagnetars Introduction The energy spectrum of cosmic rays
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High Energy amp Cosmic Ray Research Ctr North Bengal University TeV Neutrinos and Gamma rays from PulsarsMagnetars Introduction The energy spectrum of cosmic rays extends to extremely high energies values exceeding 10. IONIDES,BHADRA,ATCHAD / , , , , – 380001 AhmedabadZone , MavlankarHaveli,VasantChowk, Bhadra, LalDarwaja Ahmedabad - 380001 Ph.No.(ZM): 079 - 25507573 Ph.No. - 079 - 25505157, 25507901,25507902, 25506903 FaxNo. - 079 Sonaram Chutiya Tr. by Arunava Gupta --- For the original paper in Assamese, click here . http://www.atributetosankaradeva.org/bhakti_ratnakarara_adharat_eka_sarana_tattva_trans.pdf http://www. IONIDES,BHADRA,ATCHAD North Bengal University. TeV Neutrinos and Gamma rays from Pulsars/Magnetars. Introduction. The energy spectrum of cosmic rays extends to extremely high energies, values exceeding 10. 20. . eV. .. The origin of the cosmic rays and the mechanism responsible for acceleration of cosmic rays to such high energies .
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