lucasgautheron/CosmologyWebsite

Inhomogeneous cosmology

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This needs unification and pre-thinking. This is the last big piece before the first public release.

  • Origin of perturbations
  • Physics of the perturbations : how they grow etc ? Transfer function. P(k) -> ?
    Need the basic equations. Linear regime only ? Also need to account for DM, baryons, photons.
  • Observables : CMB TT power spectrum, galaxy 2-point correlation function, P(k) residuals.
  • Experiments : WMAP/Planck, SDSS/BOSS etc.

Appendices :

  • CMB
  • CMB power spectrum
  • Baryon acoustic oscillations
  • One for perturbations growth ?

Modern Cosmology : Scott Dodelson 978-0122191411