Astr 596 PC | Lecture 32 | Spring 2010
Astronomy 596 PC
Lecture 32, April 12
Spring 2010
Lecture Notes:
pdf file
The Large-Scale Structure of the Universe
Quantifying Cosmic Density Fields
density contrast
Fourier expansion
power spectrum defined
power spectrum observed
SDSS galaxies:
pretty pictures
and illustrated
density fluctuation spectrum
;
paper
and plots of
power spectrum
and
rms amplitude
correlation function: SDSS
galaxies
plot
,
clusters
plot
Gaussian fluctuations
Growth of Cosmological Perturbations: Linear Theory
Jeans analysis in non-expanding background
Perturbation in expanding FLRW background
Unstable modes, linear growth factor
Lecture Archive
Brian D. Fields
Last modified: Tue Apr 6 12:48:00 CDT 2010