Cosmology with Dark Sirens - Attempting to Solve the Hubble Constant Tension

Cosmology with Dark Sirens - Attempting to Solve the Hubble Constant Tension

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

The impact of incompleteness

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9 of 18

The impact of incompleteness

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Cosmology with Dark Sirens - Attempting to Solve the Hubble Constant Tension

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  1. 1 Intro
  2. 2 Outline
  3. 3 Why use gravitational waves for cosmology?
  4. 4 Cosmology with standard sirens
  5. 5 A Bayesian approach
  6. 6 GW selection effects
  7. 7 An example with 250 (mock) binary neutron stara
  8. 8 What if the host galaxy is not in the catalogue?
  9. 9 The impact of incompleteness
  10. 10 Measuring the Hubble constant with real data
  11. 11 Probability that the host galaxy is in the catalogu
  12. 12 The problem with real galaxy catalogues
  13. 13 Pixelating the analysis
  14. 14 Impact of pixelation on a single event
  15. 15 How much does pixelation improve things?
  16. 16 What is the mass distribution of the BBH popu.
  17. 17 Correlation between population and cosmolog. parameters
  18. 18 Cosmology results from GWTC-3

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