Yaroslavl State University
نویسندگان
چکیده
Neutrino transitions ν → νγ, ν → νe + e − in a strong magnetic field as a possible origin of cosmological γ-burst Abstract The high energy neutrino transitions with the photon and electron-positron pair creation in a strong magnetic field in the framework of the Standard Model are investigated. The process probabilities and the mean values of the neutrino energy and momentum loss are presented. The asymmetry of outgoing neutrinos, as a possible source of sufficient recoil " kick " velocity of a remnant and the emission of e + e −-pairs and γ-quanta in a " polar cap " region of a remnant, as a possible origin of cosmological γ-burst are discussed.
منابع مشابه
Open Problems in Discrete and Computational Geometry
H. Edelsbrunner1, A. Ivanov2 and R. Karasev3 Institute of Science and Technology Austria, Yaroslavl State University Moscow State University, Yaroslavl State University Moscow Institute of Physics and Technology, Yaroslavl State University e-mail: [email protected], [email protected], [email protected] получена 22 ноября 2006 Ключевые слова: Discrete and Computational Geometry, Computation...
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