Fall 2009
Astronomy 596/496 NPA
Oct 7
Lecture 19
Lecture Notes:
pdf file
BBN: Theory vs Observations
Predictions:
Schramm plot
(
Cyburt, Fields, & Olive 2003
)
Concordance
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
(
CFO 2003
)
BBN: Beyond the Standard Model
Standard BBN assumptions
Neutrino counting:
light element
sensitivity
to neutrino number
constraints on neutrino number from
helium-4 and/or deuterium
Lecture Archive
Brian D. Fields
Last modified: Wed Oct 7 12:22:53 CDT 2009