Astr 507 | Lecture 26 | Spring 2014
Astronomy 507
Lecture 26, March 21
Spring 2014
Lecture Notes:
pdf file
BBN:
Theory
vs
Observations
Predictions:
Schramm plot
(
BDF 2011
)
Concordance?
(
BDF, Molaro, & Sarkar 2013
)
BBN: Implications
baryon density
dark matter: two kinds!
baryonic dark matter: e.g., hot gas in
collapsed structures
and
intergalactic gas
;
MACHOs
(well,
probably not MACHOs
)
non-baryonic dark matter
BBN in Light of the CMB
Overview:
BBN+CMB Schramm plot
Standard BBN: Light element
CMB predictions vs observations
(update to
CFO 2008
)
BBN Beyond the Standard Model
relaxing and testing assumptions
counting relativistic degrees of freedom: the effective number of neutrinos (
Steigman, Schramm, and Gunn 1977
)
Lecture Archive
Brian D. Fields
Last modified: Fri Mar 21 12:47:01 CDT 2014