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Binary Neutron Star Mergers - IPAM at UCLA
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- 1 Intro
- 2 Open questions
- 3 Whisky
- 4 Neutron star merger evolution
- 5 Merger phase
- 6 Dynamical mass ejection
- 7 Dynamical and secular ejecta
- 8 Disk formation II
- 9 Prompt collapse
- 10 Multimessenger PE
- 11 Equation of state constraints
- 12 Multimessenger constraints
- 13 Early postmerger evolution
- 14 Postmerger peak frequency
- 15 Postmerger amplitude
- 16 QCD phase transitions
- 17 Long-term evolution
- 18 Spiral-wave wind (1)
- 19 Spiral-wave wind (11)
- 20 Challenges
- 21 GRAthena++
- 22 Conclusions