PPT-Leptonic
Author : tatyana-admore | Published Date : 2015-11-15
neutrinos Arunava Bhadra High Energy amp Cosmic Ray Research Ctr North Bengal University My collaborators Prabir Banik and Biplab Bijay The era of neutrino astronomy
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neutrinos Arunava Bhadra High Energy amp Cosmic Ray Research Ctr North Bengal University My collaborators Prabir Banik and Biplab Bijay The era of neutrino astronomy ing the Universe. Rosner Univ Chicago and S Stone Syracuse Univ We review the physics of purely leptonic decays of and pseudoscalar mesons The measured decay rates are related to the product of the relevant weakintera ction based CKM matrix element of the constituen S.P. Reynolds et al.. Martin, Tseng Chao . Hsiung. 2013/12/18. Which contents I will cover…. Shell Supernova Remnants: Obliquity Dependence, and . Summary!. Magnetic Fields in Pulsar-Wind Nebulae.. Neutrino Oscillations. Shun Zhou. KTH Royal Institute of Technology, Stockholm. in collaboration with T. . Ohlsson. & H. Zhang . Phys. Rev. D 87 (2013) 013012. Phys. Rev. D 87 (2013) 053006. Phys. Rev. D 88 (2013) 013001. molecular. . clouds. Armand Fiasson. LAPP - . Annecy-le-vieux. Where. . CRs. . originate. ?. The . usual. suspects up to the . knee. are . s. upernova . remnants. (. SNRs. ). Diffusive . shock. Variability of . Blazars. Markus . B. öttcher. North-West University. Potchefstroom. South Africa. 0. Blazars. Class of AGN consisting of . BL. Lac objects and gamma-ray bright qu. asars. . Rapidly (often intra-day) variable. Markus . B. öttcher. North-West University. Potchefstroom, South . Africa. 0. Most of this work done by:. Haocheng. Zhang. . (Ohio University & Los Alamos). Leptonic. . Blazar. . Model. Relativistic jet outflow with .
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