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1 | (2) |
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2 Solar Structure and Evolution |
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3 | (66) |
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2.1 Equations of Stellar Structure and Evolution |
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3 | (15) |
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2.1.1 Mechanical Structure |
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3 | (2) |
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2.1.2 Energy Conservation and Transport |
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5 | (1) |
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2.1.2.1 Energy Transport by Radiation and Conduction |
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5 | (2) |
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2.1.2.2 Criterion for Dynamical Instability |
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7 | (2) |
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2.1.2.3 Energy Transport: Convection |
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9 | (2) |
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2.1.3 Changes in Chemical Composition |
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11 | (1) |
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2.1.3.1 Convective Mixing |
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11 | (1) |
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2.1.3.2 Changes in Chemical Composition: Atomic Diffusion |
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12 | (3) |
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2.1.3.3 Changes in Chemical Composition: Nuclear Reactions |
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15 | (1) |
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2.1.3.4 Changes in Chemical Composition: Putting Everything Together |
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16 | (1) |
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2.1.4 Full Set of Equations and Boundary Conditions |
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17 | (1) |
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18 | (13) |
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18 | (3) |
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2.2.2 Radiative Opacities |
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21 | (4) |
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2.2.3 Nuclear Reaction Rates |
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25 | (6) |
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2.3 Calibrating Standard Solar Models |
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31 | (5) |
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2.3.1 Observational Constraints |
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31 | (1) |
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2.3.1.1 Age, Mass, Radius, and Luminosity |
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31 | (1) |
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2.3.1.2 Surface Composition |
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32 | (3) |
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2.3.2 Adjusting the Free Parameters |
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35 | (1) |
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2.4 Standard Solar Models |
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36 | (6) |
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2.4.1 Previous and Future Evolution |
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36 | (3) |
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2.4.2 The Sun Today: An Overview |
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39 | (3) |
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42 | (6) |
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48 | (6) |
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48 | (3) |
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2.6.2 Global Structure Inversions |
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51 | (2) |
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53 | (1) |
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2.7 Solar Abundance Problem |
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54 | (4) |
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2.8 Uncertainties in SSMs |
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58 | (4) |
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2.8.1 Uncertainties in SSM Inputs |
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58 | (1) |
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2.8.1.1 Nuclear Reaction Rates |
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58 | (1) |
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2.8.1.2 Microscopic Diffusion |
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59 | (1) |
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2.8.1.3 Radiative Opacities |
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59 | (1) |
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2.8.1.4 Solar Radius, Luminosity, and Age |
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59 | (1) |
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2.8.1.5 Solar Composition |
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59 | (1) |
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2.8.1.6 Equation of State |
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60 | (1) |
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2.8.2 Global Uncertainties in SSMs |
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60 | (1) |
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2.8.2.1 Nuclear Reaction Rates |
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61 | (1) |
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2.8.2.2 Constitutive Physics |
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61 | (1) |
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2.8.2.3 Element Abundances |
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62 | (1) |
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2.9 Solar Models Beyond the SSM |
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62 | (7) |
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2.9.1 Nonstandard Solar Physics |
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63 | (2) |
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2.9.2 Nonstandard Particle Physics |
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65 | (4) |
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69 | (70) |
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3.1 Neutrinos in the Standard Model |
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69 | (6) |
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3.2 Neutrino Oscillations |
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75 | (5) |
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80 | (4) |
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3.4 Neutrino Oscillation Experiments |
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84 | (25) |
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3.4.1 Atmospheric Neutrinos |
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84 | (8) |
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3.4.2 Long Baseline Accelerator Neutrinos |
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92 | (5) |
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3.4.2.1 Long Baseline Experiments and θ13 |
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97 | (3) |
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100 | (9) |
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3.5 Conclusions and Open Questions |
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109 | (30) |
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3.5.1 What Is the Absolute Neutrino Mass Scale? |
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111 | (9) |
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3.5.2 Are Neutrinos Majorana or Dirac Particles? |
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120 | (7) |
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3.5.3 What Is the Neutrino Mass Ordering and How Large Is CP-δ? |
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127 | (8) |
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3.5.4 Are There Sterile Neutrinos? |
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135 | (4) |
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4 Solar Neutrino Experiments |
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139 | (56) |
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139 | (2) |
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141 | (4) |
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145 | (8) |
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153 | (9) |
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162 | (7) |
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169 | (9) |
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178 | (13) |
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4.8 Summary and Open Questions |
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191 | (4) |
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5 Future Solar Neutrino Experiments |
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195 | (14) |
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196 | (3) |
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199 | (5) |
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204 | (2) |
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206 | (3) |
| References |
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209 | (12) |
| Index |
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221 | |