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Titlebook: Introduction to the Physics of Massive and Mixed Neutrinos; Samoil Bilenky Book 20101st edition Springer-Verlag Berlin Heidelberg 2010 Bey

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书目名称Introduction to the Physics of Massive and Mixed Neutrinos
编辑Samoil Bilenky
视频video
概述written by one of the pioneers in the field of modern neutrino physics (Bruno Pontecorvo Prize in 2002)..self contained introduction useful for a self-study guide.integrates classic material and state
丛书名称Lecture Notes in Physics
图书封面Titlebook: Introduction to the Physics of Massive and Mixed Neutrinos;  Samoil Bilenky Book 20101st edition Springer-Verlag Berlin Heidelberg 2010 Bey
描述For many years neutrino was considered a massless particle. The theory of a two-componentneutrino,whichplayedacrucialroleinthecreationofthetheoryof theweakinteraction,isbasedontheassumptionthattheneutrinomassisequalto zero. We now know that neutrinos have nonzero, small masses. In numerous exp- iments with solar, atmospheric, reactor and accelerator neutrinos a new p- nomenon, neutrino oscillations, was observed. Neutrino oscillations (periodic transitionsbetweendifferent?avorneutrinos? ,? ,? )arepossibleonlyifneutrino e ? ? mass-squareddifferencesaredifferentfromzeroandsmalland?avorneutrinosare “mixed”. The discovery of neutrino oscillations opened a new era in neutrino physics: an era of investigation of neutrino masses, mixing, magnetic moments and other neutrino properties. After the establishment of the Standard Model of the el- troweak interaction at the end of the seventies, the discovery of neutrino masses was the most important discovery in particle physics. Small neutrino masses cannot be explained by the standard Higgs mechanism of mass generation. For their explanation a new mechanism is needed. Thus, small neutrino masses is the ?rst signature in particle physics of a
出版日期Book 20101st edition
关键词Beyond the standard model of particle physics; Dirac and Majorana particles; Experiment; Lepton; Neutrin
版次1
doihttps://doi.org/10.1007/978-3-642-14043-3
isbn_ebook978-3-642-14043-3Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 2010
The information of publication is updating

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Neutrino Oscillations in Vacuum,in weak decays of pions and kaons, which are produced at accelerators and in the processes of interaction of cosmic ray protons in the atmosphere, in decays of muons, products of decays of pions and kaons, in .-decays of nuclei, products of the fission of uranium and plutonium in reactors, in nuclear reactions in the sun, etc.
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Neutrino in Matter,tron density depends on the distance (as in the case of the sun) the transitions probabilities between different flavor neutrinos in matter can have resonance character (MSW effect). We will consider here in some detail the propagation of neutrino in matter.
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Neutrino and Cosmology,rly Universe, the Big Bang nucleosynthesis and the number of the light neutrinos, the limit on the sum of the neutrino masses which can be inferred from the large-scale structure of the Universe and Cosmic Microwave Background radiation data. We will also consider supernova neutrinos.
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Introduction to the Physics of Massive and Mixed Neutrinos978-3-642-14043-3Series ISSN 0075-8450 Series E-ISSN 1616-6361
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