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中微子 从粒子物理学到天文学和宇宙学 英文版PDF|Epub|txt|kindle电子书版本网盘下载
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- 邢志忠,周顺著 著
- 出版社: 杭州:浙江大学出版社
- ISBN:9787308080248
- 出版时间:2011
- 标注页数:426页
- 文件大小:67MB
- 文件页数:441页
- 主题词:中微子-英文
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图书目录
1 Neutrinos:Past,Present and Future1
1.1 Neutrinos in Nuclear and Particle Physics1
1.1.1 Pauli's Neutrino Hypothesis2
1.1.2 Weak Interactions and Neutrinos3
1.1.3 Discoveries of Neutrinos4
1.2 Neutrinos in Astronomy and Cosmology6
1.2.1 Neutrinos from Stars and Supernovae7
1.2.2 High-energy Cosmic Neutrinos9
1.2.3 Cosmic Neutrino Background10
1.3 Knowledge and Questions on Neutrinos11
1.3.1 Present Knowledge on Neutrinos12
1.3.2 Open Questions on Neutrinos14
References17
2 Neutrinos within the Standard Model21
2.1 Fundamentals of the Standard Model21
2.1.1 Gauge Symmetries21
2.1.2 Spontaneous Symmetry Breaking23
2.1.3 Renormalizability25
2.1.4 The Standard Electroweak Model28
2.2 Standard Interactions of Neutrinos32
2.2.1 Neutrino-electron Scattering34
2.2.2 Neutrino-neutrino Scattering39
2.2.3 Neutrino-nucleon Interactions40
2.3 Neutrino Propagation in a Medium43
2.3.1 Coherent Forward Scattering43
2.3.2 The Effective Potential47
2.3.3 Neutrino Self-energy Approach51
References58
3 Neutrinos beyond the Standard Model61
3.1 Experimental Evidence for Neutrino Masses61
3.1.1 Atmospheric Neutrino Oscillations62
3.1.2 Accelerator Neutrino Oscillations63
3.1.3 Solar Neutrino Oscillations64
3.1.4 Reactor Neutrino Oscillations67
3.1.5 Implications of Experimental Data69
3.2 Dirac and Majorana Neutrino Mass Terms69
3.2.1 Dirac Masses and Lepton Number Conservation71
3.2.2 Majorana Masses and Lepton Number Violation73
3.2.3 Hybrid Mass Terms and Seesaw Mechanisms75
3.3 C,P and T Properties of Fermion Fields79
3.3.1 C,P and T Transformations of Spinor Bilinears79
3.3.2 CP Violation in Quark and Lepton Sectors81
3.4 Electromagnetic Properties of Massive Neutrinos86
3.4.1 Electromagnetic Form Factors86
3.4.2 Magnetic and Electric Dipole Moments89
3.4.3 Radiative Decays of Massive Neutrinos92
3.4.4 Electromagnetic Neutrino-electron Scattering94
3.5 Lepton Flavor Mixing and CP Violation97
3.5.1 Classification of Different Parametrizations97
3.5.2 Democratic and Tri-bimaximal Mixing Patterns100
3.5.3 Rephasing Invariants and Unitarity Triangles103
3.5.4 Flavor Problems in Particle Physics105
3.6 Running Behaviors of Neutrino Mass Parameters108
3.6.1 One-loop Renormalization-group Equations109
3.6.2 Evolution of Majorana Neutrino Mass Parameters111
3.6.3 Evolution of Dirac Neutrino Mass Parameters116
References119
4 Seesaw Mechanisms of Neutrino Masses125
4.1 How to Generate Tiny Neutrino Masses125
4.1.1 Non-seesaw Mechanisms126
4.1.2 Seesaw Mechanisms128
4.1.3 The Weinberg Operator129
4.2 On the Scales of Seesaw Mechanisms133
4.2.1 Seesaw-induced Hierarchy Problem133
4.2.2 Seesaw-induced Naturalness Problem134
4.3 Seesaw Mechanisms at the TeV Scale135
4.3.1 Type-ⅠSeesaw Mechanism135
4.3.2 Type-ⅡSeesaw Mechanism137
4.3.3 Type-(Ⅰ+Ⅱ) Seesaw Mechanism138
4.3.4 Type-ⅢSeesaw Mechanism140
4.3.5 Inverse Seesaw Mechanism141
4.4 Multiple Seesaw Mechanisms142
4.4.1 Two Classes of Multiple Seesaw Mechanisms143
4.4.2 Charged-current Interactions147
4.5 Non-unitary Neutrino Mixing and CP Violation150
4.5.1 Jarlskog Invariants of CP Violation151
4.5.2 Mixing Angles and CP-violating Phases152
References155
5 Phenomenology of Neutrino Oscillations159
5.1 Neutrino Oscillations and Matter Effects159
5.1.1 Neutrino Oscillations in Vacuum160
5.1.2 Adiabatic Neutrino Oscillations in Matter164
5.1.3 Non-adiabatic Neutrino Oscillations in Matter168
5.1.4 The 3×3 Neutrino Mixing Matrix in Matter171
5.1.5 Leptonic Unitarity Triangles in Matter174
5.2 Neutrino Oscillations and Quantum Coherence177
5.2.1 A Paradox of Neutrino Oscillations178
5.2.2 The Wave-packet Approach182
5.2.3 Coherence of Cosmic Neutrinos184
5.3 Density Matrix Formulation187
5.3.1 Two-flavor Neutrino Oscillations188
5.3.2 Three-flavor Neutrino Oscillations193
5.3.3 Non-linear Evolution Equations195
5.4 Future Long-baseline Neutrino Oscillation Facilities201
5.4.1 Prospects of Accelerator Neutrino Experiments201
5.4.2 Prospects of Reactor Antineutrino Experiments206
References209
6 Neutrinos from Stars213
6.1 Stellar Evolution in a Nutshell213
6.1.1 Distance,Luminosity and Mass213
6.1.2 Basic Equations of Stellar Evolution218
6.1.3 Energy Sources of Stars223
6.1.4 The Mass-Luminosity Relation226
6.2 Neutrinos from the Sun227
6.2.1 The Standard Solar Model228
6.2.2 Proton-proton Chain and CNO Cycle230
6.2.3 Solar Neutrino Fluxes232
6.3 Experimental Detection of Solar Neutrinos233
6.3.1 Radiochemical Methods233
6.3.2 Water Cherenkov Detectors237
6.3.3 Future Solar Neutrino Experiments240
6.4 Solar Neutrino Oscillations241
6.4.1 The Solar Neutrino Problem241
6.4.2 The MSW Matter Effects242
6.4.3 Constraints on Neutrino Properties244
References245
7 Neutrinos from Supernovae249
7.1 Stellar Core Collapses and Supernova Neutrinos249
7.1.1 Degenerate Stars250
7.1.2 Core-collapse Supernovae252
7.1.3 Supernova Neutrinos254
7.2 Lessons from the Supernova 1987A256
7.2.1 Discoveries of the Neutrino Burst257
7.2.2 Constraints on Neutrino Properties259
7.2.3 The Diffuse Supernova Neutrino Background260
7.2.4 Future Supernova Neutrino Experiments262
7.3 Matter Effects on Supernova Neutrinos263
7.3.1 Neutrino Fluxes and Energy Spectra265
7.3.2 Matter Efiects in the Supernova265
7.3.3 Matter Effects in the Earth269
7.4 Collective Neutrino Flavor Conversions272
7.4.1 Equations of Motion272
7.4.2 Synchronized Neutrino Oscillations275
7.4.3 Bipolar Flavor Conversions277
7.4.4 Neutrino Spectral Splits280
7.4.5 Effects of Three Neutrino Flavors283
References285
8 Ultrahigh-energy Cosmic Neutrinos289
8.1 Possible Sources of UHE Cosmic Neutrinos289
8.1.1 The GZK Cutoff and UHE Neutrinos290
8.1.2 Astrophysical Sources of UHE Neutrinos292
8.1.3 Top-down Models and UHE Neutrinos297
8.2 Detection of UHE Cosmic Neutrinos298
8.2.1 A km3-scale UHE Neutrino Telescope299
8.2.2 Identification of UHE Neutrino Flavors300
8.2.3 Other Ways to Detect UHE Neutrinos303
8.3 Flavor Distribution of UHE Cosmic Neutrinos305
8.3.1 Flavor Issues of UHE Neutrinos305
8.3.2 Flavor Efiects in New Physics Scenarios309
8.4 Neutrinos and Multi-messenger Astronomy313
8.4.1 Cosmic Neutrinos and Z-bursts313
8.4.2 Cosmic Neutrinos and Gamma Rays315
8.4.3 Neutrinos and Gravitational Waves318
References319
9 Big Bang Nucleosynthesis and Relic Neutrinos323
9.1 Neutrinos in the Early Universe323
9.1.1 Hubble's Law and the Friedmann Equations324
9.1.2 The Energy Density of the Universe325
9.1.3 The Age and Radius of the Universe327
9.1.4 Radiation in the Early Universe329
9.1.5 Neutrino Decoupling332
9.2 Big Bang Nucleosynthesis335
9.2.1 The Neutron-to-proton Ratio336
9.2.2 Synthesis of the Light Nuclei337
9.2.3 The Baryon Density and Neutrino Species340
9.3 Possible Ways to Detect Relic Neutrinos342
9.3.1 Cosmic Neutrino Background342
9.3.2 Direct Detection of Relic Neutrinos343
References347
10 Neutrinos and Cosmological Structures349
10.1 The Cosmic Microwave Background349
10.1.1 Matter-radiation Equality349
10.1.2 Formation of the CMB351
10.1.3 Anisotropies of the CMB353
10.1.4 Neutrino Species and Masses357
10.2 Large-scale Structures and Dark Matter359
10.2.1 Inflation and Density Fluctuations360
10.2.2 LSS and Dark Matter363
10.2.3 Constraints on Neutrino Masses365
10.2.4 Sterile Neutrinos as Dark Matter369
References372
11 Cosmological Matter-antimatter Asymmetry375
11.1 Baryon Asymmetry of the Universe375
11.1.1 Constraints from Antimatter Searches376
11.1.2 Observations from the CMB and BBN378
11.2 Typical Mechanisms of Baryogenesis379
11.2.1 Sakharov Conditions379
11.2.2 Electroweak Baryogenesis380
11.2.3 GUT Baryogenesis386
11.2.4 The Affleck-Dine Mechanism387
11.2.5 Leptogenesis389
11.3 Baryogenesis via Leptogenesis390
11.3.1 Thermal or Non-thermal Production390
11.3.2 CP-violating Asymmetries392
11.3.3 Boltzmann Equations398
11.3.4 Baryon Number Asymmetry405
11.4 Recent Developments in Leptogenesis408
11.4.1 Triplet Leptogenesis408
11.4.2 Resonant Leptogenesis412
11.4.3 Soft Leptogenesis413
11.4.4 Flavor Effects415
References417
Index421