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1 | (4) |
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2 Theory of Supernova Explosions |
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5 | (44) |
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6 | (1) |
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7 | (1) |
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2.3 Gravitational Collapse and Pre-supernova Conditions |
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8 | (5) |
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2.4 Production of Neutrinos and Their Emission |
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13 | (5) |
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2.5 Shock Wave Formation and Its Eventual Stalling |
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18 | (4) |
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2.6 The Revival of the Shock Wave- the Neutrino Mechanism |
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22 | (8) |
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2.7 Multi-Dimensional Hydrodynamic Simulations and the Present Scenario |
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30 | (3) |
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2.8 The Supernova SN1987A |
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33 | (5) |
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2.9 Detection of Neutrinos from Future Supernova Events |
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38 | (11) |
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44 | (5) |
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49 | (86) |
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3.1 History and Discovery of Neutron Stars |
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49 | (2) |
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3.2 Observational Constraints on Neutron Stars |
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51 | (5) |
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51 | (1) |
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52 | (2) |
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54 | (2) |
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3.3 Compositions and Novel Phases of Neutron Stars--Crust to Core |
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56 | (1) |
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3.4 Equation of State Models of Neutron Star Matter |
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57 | (12) |
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58 | (1) |
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3.4.2 Chiral Effective Field Theory Modelse |
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59 | (1) |
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3.4.3 Phenomenological Models |
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60 | (1) |
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3.4.4 EoS Models of Matter at Sub-saturation Density |
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61 | (8) |
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3.5 Relativistic Field Theoretical Models for Dense Matter at Zero and Finite Temperatures |
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69 | (24) |
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3.5.1 Relativistic Mean Field Models |
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70 | (5) |
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3.5.2 Bose-Einstein Condensates of (Anti)kaons |
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75 | (4) |
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79 | (5) |
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3.5.4 Density Dependent Hadronic Field Theory at Finite Temperature |
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84 | (4) |
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3.5.5 Antikaon Condensation at Finite Temperature |
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88 | (2) |
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3.5.6 Nuclear Physics Constraints on EoS |
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90 | (3) |
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3.6 Tolman-Oppenheimer-olkoff Equation and Structures of Neutron Stars |
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93 | (2) |
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3.7 Stable Branch of Compact Stars Beyond Neutron Star Branch |
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95 | (3) |
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3.8 Rotating Neutron Stars, Moment of Inertia and Quadrupole Moment |
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98 | (8) |
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3.8.1 Slowly Rotating Neutron Stars |
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99 | (3) |
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3.8.2 Fully Relativistic, Nonlinear Models of Rapidly Rotating Neutron Stars |
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102 | (4) |
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3.9 Neutron Star Matter in Strongly Quantizing Magnetic Fields |
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106 | (8) |
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3.9.1 Magnetized Neutron Star Crusts |
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107 | (3) |
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3.9.2 Dense Matter in Strong Magnetic Fields |
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110 | (4) |
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3.10 EoS Tables for Supernova and Binary Neutron Star Merger Simulations |
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114 | (21) |
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122 | (13) |
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4 Binary Neutron Star Mergers |
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135 | (34) |
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4.1 Gravitational Waves as New Window into Neutron Stars |
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135 | (2) |
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4.2 First Binary Neutron Star Merger GW170817 and Multimessenger Astrophysics |
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137 | (1) |
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4.3 Tidal Deformability, Love Number, and EoS |
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138 | (5) |
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4.4 I-Love-Q Universal Relations |
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143 | (3) |
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4.5 Inspiral Phase of BNS Merger, Tidal Deformability, and Cold EoS |
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146 | (4) |
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4.6 Neutron Star Radius Determination from Tidal Deformability |
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150 | (6) |
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4.7 Hot and Neutrino-Trapped Merger Remnants and Finite Temperature EoSs |
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156 | (13) |
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4.7.1 Fate of BNS Merger Remnants |
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156 | (1) |
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4.7.2 Upper Bound on Maximum Mass of Neutron Stars from GW170817 |
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157 | (3) |
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4.7.3 Finite Temperature EoSs and Imprints of Exotic Matter in GW Signals |
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160 | (2) |
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162 | (7) |
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5 Synthesis of Heavy Elements in the Universe |
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169 | (34) |
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5.1 Different Modes of Nucleosynthesis: The s-, the r-, and the p-Processes |
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169 | (11) |
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173 | (5) |
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178 | (2) |
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180 | (1) |
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5.2 Conditions for Production of Elements by the r-Process and the Sites |
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180 | (7) |
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5.2.1 The Waiting-Point Nuclei |
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180 | (1) |
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181 | (1) |
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182 | (1) |
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5.2.4 Conditions Needed for the r-Process |
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182 | (2) |
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5.2.5 The Collapse of Massive Stars as Site for the r-Process |
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184 | (2) |
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5.2.6 Neutron Star-Neutron Star/Black Hole Merger as Site for the r-Process |
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186 | (1) |
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5.3 Inputs for Nuclear Modelling of the r-Process |
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187 | (4) |
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5.3.1 Nuclear Masses/Binding Energies |
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187 | (1) |
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188 | (2) |
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5.3.3 Neutron Capture Rates |
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190 | (1) |
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5.4 Electromagnetic Counterpart of GW170817 and Ejected Matter in BNS Merger |
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191 | (1) |
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5.5 Decompression of Ejected Neutron-Rich Matter in Lattimer and Schramm Model |
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192 | (3) |
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195 | (2) |
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5.7 Heavy Element Synthesis in Neutron-Rich Matter Ejected in GW170817 |
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197 | (6) |
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198 | (5) |
Index |
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203 | |