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内容提要:
In published papers H A Bethe and G E Brown worked out the collapse of large stars and supernova explosions. They went on to evolve binaries of compact stars, finding that in the standard scenario the first formed neutron star always went into a black hole in common envelope evolution. C J Lee joined them in the study of black hole binaries and gamma ray bursts. They found the black holes to be the fossils of the gamma ray bursts. From their properties they could reconstruct features of the burst and of the accompanying hypernova explosions.
This invaluable book contains 23 papers on astrophysics, chiefly on compact objects, written over 23 years. The papers are accompanied by illuminating commentary. In addition there is an appendix on kaon condensation which the editors believe to be relevant to the equation of state in neutron stars, and to explain why black holes are formed at relatively low masses. 目录:
Preface
Chapter 1 Equation of State in the Gravitational Collapse of Stars Chapter 2 How a Supernova Explodes Chapter 3 Accretion onto and Radiation from the Compact Objects Formed in SN 1987A Chapter 4 A Scenario for a Large Number of Low-Mass Black Holes in the Galaxy Chapter 5 Neutron Star Accretion and Binary Pulsar Formation Chapter 6 How Collapsing Stars Might Hide Their Tracks in Black Holes Chapter 7 Mystery of the Missing Star Chapter 8 Observational Constraints on the Maximum Neutron Star Mass Chapter 9 On the Formation of Low-Mass Black Holes in Massive Binary Stars Chapter 10 The Evolution of Relativistic Binary Pulsars Chapter 11 Supernova Explosions, Black Holes and Nucleon Stars Chapter 12 Evolution of Binary Compact Objects That Merge Chapter 13 Contribution of High-Mass Black Holes to Mergers of Compact Binaries Chapter 14 The Formation of High-Mass Black Holes in Low-Mass X-Ray Binaries Chapter 15 Evolution of Black Holes in the Galaxy Chapter 16 The Blandford-Znajek Process as a Central Engine for a Gamma-Ray Burst Chapter 17 A Theory of Gamma-Ray Bursts Chapter 18 Hypercritical Advection-Dominated Accretion Flow Chapter 19 Evolution of Neutron Star, Carbon-Oxygen White Dwarf Binaries Chapter 20 Formation and Evolution of Black Hole X-Ray Transient Systems Chapter 21 Formation of High-Mass X-Ray Black Hole Binaries Chapter 22 Broad and Shifted Iron-Group Emission Lines in Gamma-Ray Bursts as Tests of the Hypernova Scenario Chapter 23 Discovery of a Black Hole Mass-Period Correlation in Soft X-Ray Transients and Its Implication for Gamma-Ray Burst and Hypernova Mechanisms Commentary on Appendices A-D Appendix A Kaon Condensation in Dense Stellar Matter Appendix B Kaon Production in Heavy-Ion Collisions and Maximum Mass of Neutron Stars Appendix C K-/K+ Ratios in Relativistic Heavy-Ion Collisions Appendix D Strangeness Equilibration at GSI Energies Bibliography |