Astr 596 PC | Lecture 35 | Spring 2010
Astronomy 596 PC
Lecture 35, April 19 Spring 2010

Lecture Notes: pdf file

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

CMB Anisotropies: Observations

5-year WMAP CMB sky

Lecture Archive


Brian D. Fields
Last modified: Mon Apr 19 12:30:28 CDT 2010