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18. TOWARD UNDERSTANDING GAMMA-RAY BURSTS
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Kapitel in diesem Buch
- Frontmatter i
- OVERVIEW v
- CONTENTS vii
- PREFACE xiii
- 1. THE COSMOLOGICAL PARAMETERS 1
- 2. IN THE BEGINNING . . . 25
- 3. UNDERSTANDING DATA BETTER WITH BAYESIAN AND GLOBAL STATISTICAL METHODS 49
- 4. LARGE-SCALE STRUCTURE IN THE UNIVERSE 61
- 5. UNSOLVED PROBLEMS IN GRAVITATIONAL LENSING 93
- 6. WHAT CAN B E LEARNED FROM NUMERICAL SIMULATIONS OF COSMOLOGY 115
- 7. THE CENTERS OF ELLIPTICAL GALAXIES 137
- 8. THE MORPHOLOGICAL EVOLUTION OF GALAXIES 159
- 9. QUASARS 181
- 10. SOLAR NEUTRINOS: SOLVED AND UNSOLVED PROBLEMS 195
- 11. PARTICLE DARK MATTER 221
- 12. STARS IN THE MILKY WAY AND OTHER GALAXIES 241
- 13. SEARCHING FOR MACHOs WITH MICROLENSING 253
- 14. GLOBALLY ASYMMETRIC SUPERNOVA 269
- 15. IN AND AROUND NEUTRON STARS 281
- 16. ACCRETION FLOWS AROUND BLACK HOLES 301
- 17. THE HIGHEST ENERGY COSMIC RAYS 325
- 18. TOWARD UNDERSTANDING GAMMA-RAY BURSTS 343
Kapitel in diesem Buch
- Frontmatter i
- OVERVIEW v
- CONTENTS vii
- PREFACE xiii
- 1. THE COSMOLOGICAL PARAMETERS 1
- 2. IN THE BEGINNING . . . 25
- 3. UNDERSTANDING DATA BETTER WITH BAYESIAN AND GLOBAL STATISTICAL METHODS 49
- 4. LARGE-SCALE STRUCTURE IN THE UNIVERSE 61
- 5. UNSOLVED PROBLEMS IN GRAVITATIONAL LENSING 93
- 6. WHAT CAN B E LEARNED FROM NUMERICAL SIMULATIONS OF COSMOLOGY 115
- 7. THE CENTERS OF ELLIPTICAL GALAXIES 137
- 8. THE MORPHOLOGICAL EVOLUTION OF GALAXIES 159
- 9. QUASARS 181
- 10. SOLAR NEUTRINOS: SOLVED AND UNSOLVED PROBLEMS 195
- 11. PARTICLE DARK MATTER 221
- 12. STARS IN THE MILKY WAY AND OTHER GALAXIES 241
- 13. SEARCHING FOR MACHOs WITH MICROLENSING 253
- 14. GLOBALLY ASYMMETRIC SUPERNOVA 269
- 15. IN AND AROUND NEUTRON STARS 281
- 16. ACCRETION FLOWS AROUND BLACK HOLES 301
- 17. THE HIGHEST ENERGY COSMIC RAYS 325
- 18. TOWARD UNDERSTANDING GAMMA-RAY BURSTS 343