Growth of Cosmological Perturbations: Newtonian Linear Theory
- Jeans analysis in non-expanding background
- Perturbation in expanding FLRW background
- Unstable modes, linear growth factor
Growth of Cosmological Perturbations: Sketch of Relativistic Theory
Linear Pertrubation Growth: Baryons vs Dark Matter
CMB Anisotropies
CMB Anisotropies: Theory
- baryon-photon plasma in DM potential
- acoustic oscillations and acoustic peaks
illustrations of idealized cases in real (non-k) space
- effect of cosmology and parameter determination
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