Neutrinos in particle physics, astronomy and cosmology:
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Hangzhou [u.a.]
Zhejiang Univ. Press
2011
|
| Schriftenreihe: | Advanced topics in science and technology in China
|
| Schlagworte: | |
| Online-Zugang: | Inhaltstext Inhaltsverzeichnis |
| Beschreibung: | XIV, 426 S. Ill., graph. Darst. |
| ISBN: | 9783642175596 3642175597 9787308080248 |
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Datensatz im Suchindex
| _version_ | 1805096199521304576 |
|---|---|
| adam_text |
Titel: Neutrinos in particle physics, astronomy and cosmology
Autor: Xing, Zhi-Zhong
Jahr: 2011
Contents
Neutrinos: Past, Present and Future. 1
1.1 Neutrinos in Nuclear and Particle Physics. 1
1.1.1 Pauli's Neutrino Hypothesis. 2
1.1.2 Weak Interactions and Neutrinos. 3
1.1.3 Discoveries of Neutrinos. 4
1.2 Neutrinos in Astronomy and Cosmology. 6
1.2.1 Neutrinos from Stars and Supernovae. 7
1.2.2 High-energy Cosmic Neutrinos. 9
1.2.3 Cosmic Neutrino Background. 10
1.3 Knowledge and Questions on Neutrinos . 11
1.3.1 Present, Knowledge on Neutrinos. 12
1.3.2 Open Questions on Neutrinos. 14
References. 17
Neutrinos within the Standard Model. 21
2.1 Fundamentals of the Standard Model. 21
2.1.1 Gauge Symmetries . 21
2.1.2 Spontaneous Symmetry Breaking. 23
2.1.3 Renormalizability . 25
2.1.4 The Standard Electroweak Model . 28
2.2 Standard Interactions of Neutrinos. 32
2.2.1 Neutrino-electron Scattering. 34
2.2.2 Neutrino-neutrino Scattering. 39
2.2.3 Neutrino-nucleon Interactions. 40
2.3 Neutrino Propagation in a Medium. 43
2.3.1 Coherent Forward Scattering. 43
2.3.2 The Effective Potential. 47
2.3.3 Neutrino Self-energy Approach. 51
References. 58
3 Neutrinos beyond the Standard Model . 61
3.1 Experimental Evidence for Neutrino Masses. 61
3.1.1 Atmospheric Neutrino Oscillations. 62
3.1.2 Accelerator Neutrino Oscillations. 63
3.1.3 Solar Neutrino Oscillations. 64
3.1.4 Reactor Neutrino Oscillations. 67
3.1.5 Implications of Experimental Data . 69
3.2 Dirac and Majorana Neutrino Mass Terms. 69
3.2.1 Dirac Masses and Lepton Number Conservation. 71
3.2.2 Majorana Masses and Lepton Number Violation. 73
3.2.3 Hybrid Mass Terms and Seesaw Mechanisms. 75
3.3 C, P and T Properties of Fermion Fields . 79
3.3.1 C, P and T Transformations of Spinor Bilinears. 79
3.3.2 CP Violation in Quark and Lepton Sectors. 81
3.4 Electromagnetic Properties of Massive Neutrinos. 86
3.4.1 Electromagnetic Form Factors . 86
3.4.2 Magnetic and Electric Dipole Moments. 89
3.4.3 Radiative Decays of Massive Neutrinos. 92
3.4.4 Electromagnetic Neutrino-electron Scattering. 94
3.5 Lepton Flavor Mixing and CP Violation. 97
3.5.1 Classification of Different Parametrizations. 97
3.5.2 Democratic and Tri-bimaximal Mixing Patterns. 100
3.5.3 Rephasing Invariants and Unitarity Triangles. 103
3.5.4 Flavor Problems in Particle Physics. 105
3.6 Running Behaviors of Neutrino Mass Parameters. 108
3.6.1 One-loop Renormalization-group Equations. 109
3.6.2 Evolution of Majorana Neutrino Mass Parameters . Ill
3.6.3 Evolution of Dirac Neutrino Mass Parameters. 116
References. 119
4 Seesaw Mechanisms of Neutrino Masses.125
4.1 How to Generate Tiny Neutrino Masses.125
4.1.1 Non-seesaw Mechanisms.126
4.1.2 Seesaw Mechanisms.128
4.1.3 The Weinberg Operator.129
4.2 On the Scales of Seesaw Mechanisms.133
4.2.1 Seesaw-induced Hierarchy Problem.133
4.2.2 Seesaw-induced Naturalness Problem.134
4.3 Seesaw Mechanisms at the TeV Scale .135
4.3.1 Type-I Seesaw Mechanism.135
4.3.2 Type-II Seesaw Mechanism.137
4.3.3 Type-(I-f-II) Seesaw Mechanism.138
4.3.4 Type-Ill Seesaw Mechanism.140
4.3.5 Inverse Seesaw Mechanism.141
4.4 Multiple Seesaw Mechanisms.142
4.4.1 Two Classes of Multiple Seesaw Mechanisms.143
4.4.2 Charged-current Interactions.147
4.5 Non-unitary Neutrino Mixing and CP Violation.150
4.5.1 Jarlskog Invariants of CP Violation.151
4.5.2 Mixing Angles and CP-violating Phases.152
References.155
Phenomenology of Neutrino Oscillations.159
5.1 Neutrino Oscillations and Matter Effects.159
5.1.1 Neutrino Oscillations in Vacuum.160
5.1.2 Adiabatic Neutrino Oscillations in Matter.164
5.1.3 Non-adiabatic Neutrino Oscillations in Matter.168
5.1.4 The 3x3 Neutrino Mixing Matrix in Matter .171
5.1.5 Leptonic Unitarity Triangles in Matter.174
5.2 Neutrino Oscillations and Quantum Coherence.177
5.2.1 A Paradox of Neutrino Oscillations.178
5.2.2 The Wave-packet Approach.182
5.2.3 Coherence of Cosmic Neutrinos .184
5.3 Density Matrix Formulation.187
5.3.1 Two-flavor Neutrino Oscillations.188
5.3.2 Three-flavor Neutrino Oscillations.193
5.3.3 Non-linear Evolution Equations.195
5.4 Future Long-baseline Neutrino Oscillation Facilities.201
5.4.1 Prospects of Accelerator Neutrino Experiments.201
5.4.2 Prospects of Reactor Antineutrino Experiments.206
References.209
Neutrinos from Stars.213
6.1 Stellar Evolution in a Nutshell.213
6.1.1 Distance, Luminosity and Mass.213
6.1.2 Basic Equations of Stellar Evolution.218
6.1.3 Energy Sources of Stars.223
6.1.4 The Mass-Luminosity Relation.226
6.2 Neutrinos from the Sun.227
6.2.1 The Standard Solar Model.228
6.2.2 Proton-proton Chain and CNO Cycle.230
6.2.3 Solar Neutrino Fluxes.232
6.3 Experimental Detection of Solar Neutrinos.233
6.3.1 Radiochemical Methods.233
6.3.2 Water Cherenkov Detectors.237
6.3.3 Future Solar Neutrino Experiments.240
6.4 Solar Neutrino Oscillations.241
6.4.1 The Solar Neutrino Problem.241
6.4.2 The MSW Matter Effects.242
6.4.3 Constraints on Neutrino Properties.244
References.245
Neutrinos from Supernovae.249
7.1 Stellar Core Collapses and Supernova Neutrinos.249
7.1.1 Degenerate Stars.250
7.1.2 Core-collapse Supernovae.252
7.1.3 Supernova Neutrinos.254
7.2 Lessons from the Supernova 1987A.256
7.2.1 Discoveries of the Neutrino Burst.257
7.2.2 Constraints on Neutrino Properties.259
7.2.3 The Diffuse Supernova Neutrino Background.260
7.2.4 Future Supernova Neutrino Experiments. 262
7.3 Matter Effects on Supernova Neutrinos.263
7.3.1 Neutrino Fluxes and Energy Spectra . . 265
7.3.2 Matter Effects in the Supernova. 265
7.3.3 Matter Effects in the Earth. 269
7.4 Collective Neutrino Flavor Conversions. 272
7.4.1 Equations of Motion.272
7.4.2 Synchronized Neutrino Oscillations.275
7.4.3 Bipolar Flavor Conversions.277
7.4.4 Neutrino Spectral Splits.280
7.4.5 Effects of Three Neutrino Flavors.283
References.285
Ultrahigh-energy Cosmic Neutrinos.289
8.1 Possible Sources of UHE Cosmic Neutrinos.289
8.1.1 The GZK Cutoff and UHE Neutrinos.290
8.1.2 Astrophysical Sources of UHE Neutrinos.292
8.1.3 Top-down Models and UHE Neutrinos.297
8.2 Detection of UHE Cosmic Neutrinos.298
8.2.1 A km3-scale UHE Neutrino Telescope.299
8.2.2 Identification of UHE Neutrino Flavors.300
8.2.3 Other Ways to Detect UHE Neutrinos .303
8.3 Flavor Distribution of UHE Cosmic Neutrinos.305
8.3.1 Flavor Issues of UHE Neutrinos.305
8.3.2 Flavor Effects in New Physics Scenarios.309
8.4 Neutrinos and Multi-messenger Astronomy.313
8.4.1 Cosmic Neutrinos and Z-bursts.313
8.4.2 Cosmic Neutrinos and Gamma Rays.315
8.4.3 Neutrinos and Gravitational Waves.318
References.319
9 Big Bang Nucleosynthesis and Relic Neutrinos .323
9.1 Neutrinos in the Early Universe.323
9.1.1 Hubble's Law and the Friedmann Equations.324
9.1.2 The Energy Density of the Universe .325
9.1.3 The Age and Radius of the Universe.327
9.1.4 Radiation in the Early Universe.329
9.1.5 Neutrino Decoupling.332
9.2 Big Bang Nucleosynthesis .335
9.2.1 The Neutron-to-proton Ratio.336
9.2.2 Synthesis of the Light Nuclei.337
9.2.3 The Baryon Density and Neutrino Species.340
9.3 Possible Ways to Detect Relic Neutrinos.342
9.3.1 Cosmic Neutrino Background.342
9.3.2 Direct Detection of Relic Neutrinos.343
References.347
10 Neutrinos and Cosmological Structures.349
10.1 The Cosmic Microwave Background.349
10.1.1 Matter-radiation Equality. 349
10.1.2 Formation of the CMB. 351
10.1.3 Anisotropics of the CMB. 353
10.1.4 Neutrino Species and Masses. 357
10.2 Large-scale Structures and Dark Matter. 359
10.2.1 Inflation and Density Fluctuations.360
10.2.2 LSS and Dark Matter.363
10.2.3 Constraints on Neutrino Masses.365
10.2.4 Sterile Neutrinos as Dark Matter.369
References.372
11 Cosmological Matter-antimatter Asymmetry .375
11.1 Baryon Asymmetry of the Universe.375
11.1.1 Constraints from Antimatter Searches.376
11.1.2 Observations from the CMB and BBN.378
11.2 Typical Mechanisms of Baryogenesis.379
11.2.1 Sakharov Conditions.379
11.2.2 Electroweak Baryogenesis .380
11.2.3 GUT Baryogenesis .386
11.2.4 The Affleck-Dine Mechanism.387
11.2.5 Leptogenesis.389
11.3 Baryogenesis via Leptogenesis.390
11.3.1 Thermal or Non-thermal Production.390
11.3.2 CP-violating Asymmetries.392
11.3.3 Boltzmann Equations.398
11.3.4 Baryon Number Asymmetry.405
11.4 Recent Developments in Leptogenesis.408
11.4.1 Triplet Leptogenesis.408
11.4.2 Resonant Leptogenesis.412
11.4.3 Soft Leptogenesis.413
11.4.4 Flavor Effects.415
References.417
Index.421 |
| any_adam_object | 1 |
| author | Xing, Zhi-Zhong Zhou, Shun |
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| discipline | Physik |
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| title_short | Neutrinos in particle physics, astronomy and cosmology |
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