Astronomy 406
Lecture 36, Nov. 20
Fall 2013
Lecture Notes:
pdf file
The Cosmic Microwave Background to High Precision
the CMB sky
, normal contrast
high-contrast (1000X): CMB
dipole
higher contrast (100,000X):
COBE (1995)
WMAP
(2003):
raw
,
reduced
COBE vs WMAP
Planck: survey
animation
,
one strip
,
all sky
;
Planck vs WMAP
fluctuations vs angular scale:
WMAP power spectrum
cool movies courtesy
WMAP
,
Planck
physical
origin
of fluctuations
polarization:
from WMAP
the lensed CMB:
dark matter map
from Planck
The Nuclear Age: Primordial Nucleosynthesis
Prelude
baryons
nuclei
and
nuclear forces
Big Bang Nucleosynthesis: Theory
History
prelude:
alpha beta gamma
Alpher, Herman, and Gamow arising from Ylem
Radiation domination
Particle ingredients
Element formation:
reaction network
predictions:
Schramm plot
(
Cyburt, Fields, & Olive 2003
)
Lecture Archive
Brian D. Fields
Last modified: Wed Nov 20 10:42:38 CST 2013