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Kilonova Modeling
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Classroom Contents
Nuclear Matter EOS Constraints from Gravitational Waves by Wolfgang Kastaun
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- 1 Nuclear matter EOS constraints from GW
- 2 Outline
- 3 Inspiral Parameter Space
- 4 Impact of Parameters
- 5 Measurable EOS Aspects For GW170817 Maximum NS mass _ 1.36Mo
- 6 Model-Agnostic Study
- 7 Universal Relations Studies
- 8 Parametrization
- 9 Evidence for Tidal Effects?
- 10 EOS Model Selection Study
- 11 Implication of Remnant Type
- 12 Implication of Remnant Type Recent analysis [Shibata et al, Phys. Rev. 100 2019] Less assumptions
- 13 Kilonova
- 14 Mass ejection
- 15 Kilonova Modeling
- 16 Constraints from Kilonova
- 17 Short Gamma Ray Burst Models
- 18 Numerical Simulations
- 19 Other Avenues
- 20 Post-Merger Signal
- 21 Searching p-g effects
- 22 Appendix
- 23 Q&A
