Astr 328 April 14, 2003: Growth of perturbations in a universe with dark matter  

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Things get way easier when we add dark matter

Review on why things are hard without DM

Different examples of decoupling

Decoupling of neutrinos

Let's do structure formation with DM

WIMPs or neutrinos?

Hot dark matter

Cold Dark Matter

What can two-point correlation function tell us about initial density fluctuations?

Two-point correlation function

When does our treatment fail?

Initial power spectrum

Harrison-Zeldovich spectrum