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Titlebook: Electroweak Processes in External Active Media; Alexander Kuznetsov,Nickolay Mikheev Book 2013 Springer-Verlag Berlin Heidelberg 2013 Dira

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發(fā)表于 2025-3-21 17:20:49 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Electroweak Processes in External Active Media
編輯Alexander Kuznetsov,Nickolay Mikheev
視頻videohttp://file.papertrans.cn/307/306575/306575.mp4
概述Covers new effects of a pure magnetic field on electroweak.Focus lays on the calculation technique for electroweak processes in external active media - hot dense plasma.Useful reference for researcher
叢書名稱Springer Tracts in Modern Physics
圖書封面Titlebook: Electroweak Processes in External Active Media;  Alexander Kuznetsov,Nickolay Mikheev Book 2013 Springer-Verlag Berlin Heidelberg 2013 Dira
描述Expanding on the concept of the authors’ previous book “ElectroweakProcesses in External Electromagnetic Fields,” this new booksystematically describes the investigation methods for the effects ofexternal active media, both strong electromagnetic fields and hotdense plasma, in quantum processes. Solving the solar neutrino puzzlein a unique experiment conducted with the help of the heavy-waterdetector at the Sudbery Neutrino Observatory, along with another neutrino experiments, brings to the fore electroweak physics in an active external medium. It is effectively demonstrated that processes of neutrino interactions with active media of astrophysical objects may lead, under some physical conditions, to such interesting effects as neutrino-driven shockwave revival in a supernova explosion, a “cherry stone shooting” mechanism for pulsar natal kick, and aneutrino pulsar. It is also shown how poor estimates of particle dispersion in external active media sometimes lead to confusion. The book will appeal to graduate and post-graduate students of theoretical physics with a prior understanding of Quantum Field Theory (QFT) and the Standard Model of Electroweak Interactions, as well as to sp
出版日期Book 2013
關(guān)鍵詞Dirac Equation; Elementary Particle Processes; Hot Dense Plasma; Neutrino Interactions; Neutron Star; Par
版次1
doihttps://doi.org/10.1007/978-3-642-36226-2
isbn_softcover978-3-642-44647-4
isbn_ebook978-3-642-36226-2Series ISSN 0081-3869 Series E-ISSN 1615-0430
issn_series 0081-3869
copyrightSpringer-Verlag Berlin Heidelberg 2013
The information of publication is updating

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Sergey Libert,Razvan Chisu,Artur Luftomentum losses due to the process ., which could be essential in astrophysical applications. The process of the electron–positron pair production by neutrino in a strong magnetic field, if one more component of the external active medium which is dense plasma is taken into account, should be suppres
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Electromagnetic Interactions in External Active Media,i) via the imaginary part of the loop amplitude. We analyse also the process of the photon emission by an electron in magnetic fields which is the crossed process to the . decay. The second process considered is the electromagnetic interaction of the Dirac neutrino having a magnetic moment, with pla
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https://doi.org/10.1007/978-3-642-36226-2Dirac Equation; Elementary Particle Processes; Hot Dense Plasma; Neutrino Interactions; Neutron Star; Par
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Research Field, Subjects and Informants,nalysis of quantum processes. The transformation from one representation to another are provided which can be useful from a methodological point of view. The exact propagator for an electron in a constant uniform magnetic field as the sum over Landau levels is obtained by the direct derivation by st
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