1Neutrinos: Past， Present and Future

1.1  Neutrinos in Nuclear and Particle Physics

1.1.1  Pauli's Neutrino Hypothesis

1.1.2  Weak Interactions and Neutrinos

1.1.3  Discoveries of Neutrinos

1.2  Neutrinos in Astronomy and Cosmology

1.2.1  Neutrinos from Stars and Supernovae

1.2.2  High-energy Cosmic Neutrinos

1.2.3  Cosmic Neutrino Background

1.3  Knowledge and Questions on Neutrinos

1.3.1  Present Knowledge on Neutrinos

1.3.2  Open Questions on Neutrinos

References

2Neutrinos within the Standard Model

2.1  Fundamentals of the Standard Model

2.1.1  Gauge Symmetries

2.1.2  Spontaneous Symmetry Breaking

2.1.3  Renormalizability

2.1.4  The Standard Electroweak Model

2.2  Standard Interactions of Neutrinos

2.2.1  Neutrino-electron Scattering

2.2.2  Neutrino-neutrino Scattering

2.2.3  Neutrino-nucleon Interactions

2.3  Neutrino Propagation in a Medium

2.3.1  Coherent Forward Scattering

2.3.2  The Effective Potential

2.3.3  Neutrino Self-energy Approach

References

3  Neutrinos beyond the Standard Model

3.1  Experimental Evidence for Neutrino Masses

3.1.1  Atmospheric Neutrino Oscillations

3.1.2  Accelerator Neutrino Oscillations

    3.1.3  Solar Neutrino Oscillations

3.1.4  Reactor Neutrino Oscillations

3.1.5  Implications of Experimental Data

  3.2  Dirac and Majorana Neutrino Mass Terms

3.2.1  Dirac Masses and Lepton Number Conservation

3.2.2. Majorana Masses and Lepton Number Violation

3.2.3  Hybrid Mass Terms and Seesaw Mechanisms

  3.3  C, P and T Properties of Fermion Fields

3.3.1  C, P and T Transformations of Spinor Bilinears

3.3.2  CP Violation in Quark and Lepton Sectors

  3.4  Electromagnetic Properties of Massive
Neutrinos

3.4.1  Electromagnetic Form Factors

3.4.2  Magnetic and Electric Dipole Moments

3.4.3  Radiative Decays of Massive Neutrinos

3.4.4  Electromagnetic Neutrino-electron Scattering

  3.5  Lepton Flavor Mixing and CP Violation

3.5.1  Classification of Different Parametrizations

3.5.2  Democratic and Tri-bimaximal Mixing Patterns

3.5.3  Rephasing Invariants and Unitarity Triangles

3.5.4  Flavor Problems in Particle Physics

  3.6  Running Behaviors of Neutrino Mass
Parameters

3.6.1  One-loop Renormalization-group Equations

3.6.2  Evolution of Majorana Neutrino Mass Parameters

3.6.3  Evolution of Dirac Neutrino Mass Parameters

   References

4Seesaw Mechanisms of Neutrino Masses

  4.1  How to Generate Tiny Neutrino Masses

4.1.1  Non-seesaw Mechanisms

4.1.2  Seesaw Mechanisms

4.1.3  The Weinberg Operator

  4.2  On the Scales of Seesaw Mechanisms

4.2.1  Seesaw-induced Hierarchy Problem

4.2.2  Seesaw-induced Naturalness Problem

  4.3  Seesaw Mechanisms at the TeV Scale

4.3.1  Type-I Seesaw Mechanism

4.3.2  Type-II Seesaw Mechanism

4.3.3  Type-(I+II) Seesaw Mechanism

4.3.4  Type-III Seesaw Mechanism

4.3.5  Inverse Seesaw Mechanism

  4.4  Multiple Seesaw Mechanisms

……

5Phenomenology of Neutrino Oscillations

6Neutrinos from Stars

7  Neutrinos from Supernovae

8Ultrahigh-energy Cosmic Neutrinos

9  Big Bang Nucleosynthesis and Relic Neutrinos

10Neutrinos and Cosmological Structures

11  Cosmological Matter-antimatter Asymmetry

Index