Astronomy 406
Lecture 38, Dec. 2
Fall 2013
Lecture Notes:
pdf file
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
)
BBN: Observations
Problem: pollution; solution: trace evolution
the circle, the
circle of life
Helium-4
dwarf (blue compact) galaxy I Zwicky 18:
UV
,
optical (HST)
spectra
(
Izotov et al 1999
)
Deuterium
QSO absorption line systems:
typical spectra
deuterium system HS 0105+1619 (
O'Meara et al 2001
):
spectrum overview
,
hydrogen and deuterium lines
Lithium
extreme Pop II (halo) stars
Helium-3
BBN: Theory vs Observations
Predictions:
Schramm plot
(
Cyburt, Fields, & Olive 2003
)
Concordance
BBN: Implications
cosmic baryon inventory
baryonic dark matter
hot intergalatic gas:
predicted
and maybe
observed
?
non-baryonic dark matter
particle physics
: the universe as the
poor man's accelerator!
Lecture Archive
Brian D. Fields
Last modified: Mon Dec 2 10:40:24 CST 2013