Structure Formation Continued

• Why we need dark matter
  
• Dark Matter and Perturbation Growth
• Dark Matter and Perturbation Growth 2
• Plot of delta(B)/delta(D) as a fn of log z
  
• Forms of Dark Matter
• Hot Dark Matter
• Structure Growth - Hot vs Cold
• Evolution of the Power Spectrum
• Early Evolution of the Power Spectrum (Figure)
  
• Nonlinear effects on the correlation function
  
• Post Recombination Evolution of the Power Spectrum
  
• Galaxy Biasing
  
• Galaxy Biasing Figure