Gravitational Wave Paleontology: Understanding Black Hole and Neutron Star Mergers in the Big Data Era

Gravitational Wave Paleontology: Understanding Black Hole and Neutron Star Mergers in the Big Data Era

MonashPhysicsAndAstronomy via YouTube Direct link

Introduction

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1 of 30

Introduction

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Classroom Contents

Gravitational Wave Paleontology: Understanding Black Hole and Neutron Star Mergers in the Big Data Era

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  1. 1 Introduction
  2. 2 The Tipping Point
  3. 3 How do systems form
  4. 4 Simulation
  5. 5 Merger Rates
  6. 6 Review Paper
  7. 7 Uncertainty
  8. 8 What now
  9. 9 Quantifying uncertainties
  10. 10 Different types of uncertainties
  11. 11 Supernova models
  12. 12 Binary black holes
  13. 13 Binary stars
  14. 14 Binary blackholes
  15. 15 Merger shapes
  16. 16 Spins
  17. 17 Spin fraction
  18. 18 Formation channels
  19. 19 Information channels
  20. 20 Transients
  21. 21 Computational costs
  22. 22 Normalizing flows
  23. 23 Improving Stellar Evolution codes
  24. 24 Comparing codes
  25. 25 We need you
  26. 26 We are not there
  27. 27 Uncertainty is common
  28. 28 Support Structures
  29. 29 Takeaways
  30. 30 The Rose Report

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