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[null,"1.","Record Nr.",null,"UNINA9910552988703321"]
[null,null,"Autore",null,"Zuber K."]
[null,null,"Titolo",null,"Neutrino physics / / Kai Zuber"]
[null,null,"Pubbl/distr/stampa",null,"Taylor & Francis, 2020"]
[{"$nulls":4},"Boca Raton, FL : , : CRC Press, , 2020"]
[{"$nulls":4},"©2020"]
[null,null,"ISBN",null,"9781351764575"]
[{"$nulls":4},"1351764578"]
[{"$nulls":4},"9781315195612"]
[{"$nulls":4},"1315195615"]
[{"$nulls":4},"9781351764582"]
[{"$nulls":4},"1351764586"]
[null,null,"Edizione",null,"[Third edition.]"]
[null,null,"Descrizione fisica",null,"1 online resource (550 pages)"]
[null,null,"Collana",null,"Series in high energy physics, cosmology & gravitation"]
[null,null,"Disciplina",null,"539.7/215"]
[null,null,"Soggetti",null,"Neutrinos"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Nota di bibliografia","Includes bibliographical references and index."]
[null,null,"Nota di contenuto",null,"Cover -- Half Title -- Series Page -- Title Page -- Copyright Page -- Table of Contents -- Preface to the First Edition -- Preface to the Second Edition -- Preface to the Third Edition -- Notation -- 1: Important Historical Experiments -- 1.1 The Birth of the Neutrino -- 1.2 Nuclear Recoil Experiment by Rodeback and Allen -- 1.3 Discovery of the Neutrino by Cowan and Reines -- 1.4 Difference between ve and ve and solar neutrino detection -- 1.5 Discovery of Parity Violation in Weak Interactions -- 1.6 Direct Measurement of the Helicity of the Neutrino -- 1.7 Experimental Proof That Vμ is Different from Ve -- 1.8 Discovery of Weak Neutral Currents -- 1.9 Discovery of the Weak W± and Z0 Gauge Bosons -- 1.10 Observation of Neutrinos from SN 1987A -- 1.11 Number of Neutrino Flavours from the Width of the Z0 -- 1.12 Further Milestones in the Last 20 Years -- 2: Properties of Neutrinos -- 2.1 Helicity and Chirality -- 2.2 Charge Conjugation -- 2.3 Parity Transformation -- 2.4 Dirac and Majorana Mass Terms -- 2.4.1 Generalization to n Flavours -- 2.5 Lepton Number -- 2.5.1 Experimental Status of Lepton Flavour and Number Violation -- 3: The Standard Model of Particle Physics -- 3.1 The V-A Theory of the Weak Interaction -- 3.2 Gauge Theories -- 3.2.1 The Gauge Principle -- "]
[{"$nulls":4},"3.2.2 Global Symmetries -- 3.2.3 Local (=Gauge) Symmetries -- 3.2.4 Non-Abelian Gauge Theories (= Yang-Mills Theories) -- 3.3 The Glashow-Weinberg-Salam Model -- 3.3.1 Spontaneous Symmetry Breaking and the Higgs Mechanism -- 3.3.2 The CKM Mass Matrix -- 3.3.3 CP Violation -- 3.3.4 CPT and T Violation -- 3.4 Experimental Determination of Fundamental Parameters -- 3.4.1 Measurement of the Fermi Constant GF -- 3.4.2 Neutrino-Electron Scattering and the Coupling Constants gV and gA -- 3.4.2.1 Theoretical considerations -- 3.4.2.2 Vμe-Scattering -- 3.4.2.3 Vee and Vee-Scattering."]
[{"$nulls":4},"3.4.2.4 Neutrino Tridents -- 3.4.3 Measurement of the Weinberg Angle -- 3.4.4 Measurement of the Gauge Boson Masses mW and mZ -- 3.4.5 The Discovery of the Higgs Boson -- 4: Neutrinos as a Probe of Nuclear Structure -- 4.1 Neutrino Beams -- 4.1.1 Conventional Beams -- 4.1.1.1 Narrow-Band Beams -- 4.1.1.2 Wide-Band Beams -- 4.1.2 VT Beams -- 4.1.3 Off-Axis Superbeams -- 4.1.4 Alternative Neutrino Beams -- 4.2 Neutrino Detectors -- 4.2.1 OPERA -- 4.2.2 NOVA -- 4.2.3 T2K -- 4.2.4 DUNE -- 4.3 Total Cross-Section for Neutrino-Nucleon Scattering -- 4.4 Coherent Elastic Neutrino-Nucleus Scattering -- 4.5 Quasi-Elastic Neutrino-Nucleon Scattering -- 4.5.1 Quasi-Elastic CC Reactions -- 4.5.2 Quasi-Elastic NC Reactions -- 4.6 Kinematics of Deep Inelastic Scattering -- 4.7 Coherent, Resonant and Diffractive Production -- 4.8 Structure Function of Nucleons -- 4.9 the Quark-Parton Model, Parton Distribution Functions -- 4.9.1 Deep Inelastic Neutrino Proton Scattering -- 4.9.1.1 QCD effects -- 4.10 y Distributions and Quark Content from Total Cross-Sections -- 4.10.1 Sum Rules -- 4.11 Charm Physics -- 4.12 Neutral Current Reactions -- 4.13 Neutrino Cross-Section on Nuclei -- 5: Neutrino Masses and Physics Beyond the Standard Model -- 5.1 Running Coupling Constants -- 5.2 The Minimal SU(5) Model -- 5.2.1 Proton Decay -- 5.3 The SO(10) Model -- 5.3.1 Left-Right Symmetric Models -- 5.4 Supersymmetry -- 5.4.1 The Minimal Supersymmetric Standard Model -- 5.4.2 R-Parity -- 5.4.3 Experimental Search for Supersymmetry -- 5.4.3.1 SUSY Signatures at High Energy Colliders -- 5.4.3.2 SUSY GUTs and Proton Decay -- 5.5 Neutrino Masses -- 5.5.1 Neutrino Masses in the Electroweak Theory -- 5.5.2 Neutrino Masses in the Minimal SU(5) Model -- 5.5.3 Neutrino Masses in the SO(10) Model and the Seesaw Mechanism -- 5.5.3.1 Almost Degenerated Neutrino Masses."]
[{"$nulls":4},"5.5.4 Neutrino Masses in SUSY and Beyond -- 5.6 Neutrino Mixing -- 6: Direct Neutrino Mass Searches -- 6.1 Fundamentals of β-Decay -- 6.1.1 Matrix Elements -- 6.1.2 Phase Space Calculation -- 6.1.3 Kurie Plot and ft-Values -- 6.2 Searches for mve -- 6.2.1 General Considerations -- 6.2.2 Searches Using Spectrometers -- 6.2.2.1 The KATRIN experiment -- 6.2.2.2 Project 8 -- 6.2.3 Alternative Searches -- 6.2.4 Kinks in β-Decay -- 6.3 Searches For mve -- 6.4 mvµ Determination from Pion Decay -- 6.5 Mass of the VT From Tau Decay -- 6.6 Electromagnetic Properties of Neutrinos -- 6.6.1 Electric Dipole Moments -- 6.6.2 Magnetic Dipole Moments -- 6.7 Neutrino Decay -- 6.7.1 Radiative Decay VH → VL + ϒ -- 6.7.2 The Decay VH → VL + e+ + e- -- 6.7.3 The Decay VH → VL + X -- 6.8 Heavy Neutrinos -- 7: Double Beta Decay -- 7.1 Introduction -- 7.2 Decay Rates -- 7.2.1 The 2V ββ Decay Rates -- 7.2.2 The 0V ββ Decay Rates -- 7.3 Nuclear Structure Effects on Matrix Elements -- 7.4 Experiments -- 7.4.1 Practical Considerations in Low-level Counting -- 7.4.2 Direct Counting Experiments -- 7.4.2.1 Semiconductor Experiments -- 7.4.2.2 Scintillator Experiments -- 7.4.2.3 Cryogenic Detectors -- 7.4.2.4 Ionization Experiments -- 7.4.3 Geochemical Experiments -- 7.4.4 Radiochemical Experiments -- 7.5 Interpretation of the Obtained Results -- 7.5.1 Effects of MeV Neutrinos -- 7.5.2 Transitions to "]
[{"$nulls":4},"Excited States -- 7.5.3 Majoron Accompanied Double β-decay -- 7.5.4 Decay Rates for SUSY-Induced 0V ββ Decay -- 7.6 Positron Decay and Electron Capture Decay Modes -- 7.7 CP Phases and Double Beta Decay -- 7.8 Generalization to Three Flavours -- 7.8.1 General Considerations -- 7.8.1.1 Muon-Positron Conversion on Nuclei -- 7.8.1.2 Processes Investigating mµµ -- 7.8.1.3 Limits on mTT from CC events at HERA -- 8: Neutrino Oscillations -- 8.1 General Formalism."]
[{"$nulls":4},"8.2 CP and T Violation in Neutrino Oscillations -- 8.3 Oscillations with Two Neutrino Flavours -- 8.4 The Case for Three Flavours -- 8.5 Experimental Considerations -- 8.6 Nuclear Reactor Experiments -- 8.6.1 Experimental Status -- 8.6.1.1 KamLAND-Measurement of θ12 -- 8.6.1.2 Double Chooz, RENO and Daya Bay-Measurement of θ13 -- 8.6.2 Geoneutrinos -- 8.7 Accelerator-Based Oscillation Experiments -- 8.8 Neutrino Oscillations in Matter -- 8.9 Future Activities - Determination of the PMNS Matrix Elements -- 8.10 New Neutrinos Beams -- 8.10.1 Off-Axis Superbeams -- 8.10.2 Muon Storage Rings - Neutrino Factories -- 9: Atmospheric Neutrinos -- 9.1 Cosmic Rays -- 9.2 Interactions Within the Atmosphere -- 9.3 Experimental Status -- 9.3.1 Super-Kamiokande -- 9.3.1.1 The Vµ/Ve Ratio -- 9.3.1.2 Zenith-Angle Distributions -- 9.3.1.3 Oscillation Analysis -- 9.4 Accelerator-Based Searches - Long-Baseline Experiments -- 9.4.1 K2K -- 9.4.2 MINOS -- 9.4.3 CERN-Gran Sasso -- 9.5 Future Experimental Plans and Ideas -- 9.5.1 INO-ICAL -- 9.5.2 Hyper-Kamiokande -- 9.5.3 THEIA -- 9.5.4 AQUA-RICH -- 10: Solar Neutrinos -- 10.1 The Standard Solar Model -- 10.1.1 Energy Production Processes in the Sun -- 10.1.2 Reaction Rates -- 10.1.3 The Solar Neutrino Spectrum -- 10.1.3.1 Standard Solar Models -- 10.1.3.2 Diffusion -- 10.1.3.3 Initial Composition -- 10.1.3.4 Opacity and Equation of State -- 10.1.3.5 Predicted Neutrino Fluxes -- 10.2 Solar Neutrino Experiments -- 10.2.1 The Chlorine Experiment -- 10.2.2 Super-Kamiokande -- 10.2.3 The Gallium Experiments -- 10.2.3.1 GALLEX -- 10.2.3.2 GNO -- 10.2.3.3 SAGE -- 10.2.4 The Sudbury Neutrino Observatory (SNO) -- 10.2.5 The Borexino Experiment -- 10.3 Theoretical Solutions-Matter Effects -- 10.3.1 Neutrino Oscillations as a Solution to the Solar Neutrino Problem -- 10.3.2 Neutrino Oscillations in Matter and the MSW Effect."]
[{"$nulls":4},"10.3.2.1 Constant Density of Electrons -- 10.3.2.2 Variable Electron Density -- 10.3.3 Experimental Signatures and Results -- 10.4 Future Potential Experiments -- 10.4.1 Real-Time Measurement of PP Neutrinos Using Coincidence Techniques -- 11: Neutrinos from Supernovae -- 11.1 Supernovae -- 11.1.1 The Evolution of Massive Stars -- 11.1.2 Energy Loss of Massive Stars Due to Neutrino Emission -- 11.1.3 The Actual Collapse Phase -- 11.2 Neutrino Emission in Supernova Explosions -- 11.2.1 The Classical Prediction -- 11.2.2 Neutrino Oscillations and Supernova Signals -- 11.2.2.1 Effects on the Prompt Ve Burst -- 11.2.2.2 Cooling Phase Neutrinos -- 11.2.2.3 Production of R-Process Isotopes -- 11.2.2.4 Neutrino Mass Hierarchies from Supernova Signals -- 11.3 Detection Methods for Supernova Neutrinos -- 11.4 Supernova 1987A -- 11.4.1 Characteristics of Supernova 1987A -- 11.4.1.1 Properties of the Progenitor Star and the Event -- 11.4.1.2 ϒ-Radiation -- 11.4.1.3 Distance -- 11.4.1.4 Summary -- 11.4.2 Neutrinos from SN 1987A -- 11.4.2.1 Possible Anomalies -- 11.4.3 Neutrino Properties from SN 1987A -- 11.4.3.1 Lifetime of the Neutrino -- 11.4.3.2 Mass of the Neutrino -- 11.4.3.3 Magnetic Moment and Electric Charge -- 11.4.3.4 Conclusion -- 11.5 Supernova Rates and Future Experiments -- 11.5.1 Diffuse Supernova Neutrino Background -- 12: Ultra-High Energetic Cosmic Neutrinos -- 12.1 Sources of High-Energy Cosmic Neutrinos -- "]
[{"$nulls":4},"12.1.1 Neutrinos Produced in Acceleration Processes -- 12.1.2 Neutrinos Produced in Annihilation or Decay of Heavy Particles -- 12.1.3 Event Rates -- 12.1.4 Neutrinos from Active Galactic Nuclei -- 12.1.5 Neutrinos from Gamma Ray Bursters -- 12.1.6 Cross-Sections -- 12.2 Detection -- 12.2.1 Water Cherenkov Detectors -- 12.2.1.1 Baikal NT-200 -- 12.2.1.2 ANTARES -- 12.2.2 Ice Cherenkov Detectors-IceCube -- 12.2.3 Multi-Messenger Approaches."]
[{"$nulls":4},"12.2.4 Gravitational Waves."]
[null,null,null,"Sommario/riassunto","When Kai Zuber's pioneering text on neutrinos was published in 2003, the author correctly predicted that the field would see tremendous growth in the immediate future. In that book, Professor Zuber provided a comprehensive self-contained examination of neutrinos, covering their research history and theory, as well as their application to particle physics, astrophysics, nuclear physics, and the broad reach of cosmology; but now to be truly comprehensive and accurate, the field's seminal reference needs to be revised and expanded to include the latest research, conclusions, and implications. Revised as needed to be equal to the research of today, Neutrino Physics, Third Edition delves into neutrino cross-sections, mass measurements, double beta decay, solar neutrinos, neutrinos from supernovae, and high-energy neutrinos, as well as entirely new experimental results in the context of theoretical models. Written to be accessible to graduate students and readers from diverse backgrounds, this edition, like the first, provides both an introduction to the field as well as the information needed by those looking to make their own contributions to it. And like the second edition, it whets the researcher's appetite, going beyond certainty to pose those questions that still need answers. Features Presents the only single-author comprehensive text on neutrino physics Includes experimental and theoretical particle physics and examines solar neutrinos and astroparticle implications Offers details on new developments and recent experiments"]