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