Gravitational-Wave Observations of Neutron-Star Mergers - IPAM at UCLA

Gravitational-Wave Observations of Neutron-Star Mergers - IPAM at UCLA

Institute for Pure & Applied Mathematics (IPAM) via YouTube Direct link

New mass distribution

23 of 26

23 of 26

New mass distribution

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Gravitational-Wave Observations of Neutron-Star Mergers - IPAM at UCLA

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  1. 1 Introduction
  2. 2 What are neutronstars
  3. 3 Orbital dynamics
  4. 4 Gravitationalwave
  5. 5 Oversimplified picture
  6. 6 Deformations
  7. 7 Waveform models
  8. 8 Universal relations
  9. 9 Equivalent waveforms
  10. 10 Descriptive bottleneck
  11. 11 Properties of matter
  12. 12 Functional forms
  13. 13 Gravitationalwave data
  14. 14 Other observations
  15. 15 Representational challenges
  16. 16 Model comparison
  17. 17 Terrestrial experiments
  18. 18 Nuclear theory
  19. 19 Comparing observations
  20. 20 Future generation observatories
  21. 21 Other ways
  22. 22 Galactic neutronstars
  23. 23 New mass distribution
  24. 24 Missing something important
  25. 25 Next generation
  26. 26 Communication

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