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Primordial nucleosynthesis redux
The abundances of D, He-3, He-4, and Li-7, are presently recalculated within the framework of primordial nucleosynthesis in the standard hot big band model, in order to estimate the primordialExpand
Primordial Nucleosynthesis in the Precision Cosmology Era
Primordial nucleosynthesis probes the Universe during its early evolution. Given the progress in exploring the constituents, structure, and recent evolution of the Universe, it is timely to reviewExpand
PRIMORDIAL NUCLEOSYNTHESIS: SUCCESSES AND CHALLENGES
Primordial nucleosynthesis provides a probe of the Universe during its early evolution. Given the progress exploring the constituents, structure, and recent evolution of the Universe, it is timely toExpand
Primordial helium and the cosmic background radiation
The products of primordial nucleosynthesis, along with the cosmic microwave background (CMB) photons, are relics from the early evolution of the Universe whose observations probe the standard modelExpand
Inflationary cosmology
The Very Early Universe.Edited by G.W. Gibbons, S.W. Hawking and S.T.C. Siklos. Cambridge University Pres: 1983. Pp.480. £25, $49.50.
Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
If dark matter (DM) is a weakly interacting massive particle (WIMP) that is a thermal relic of the early Universe, then its total self-annihilation cross section is revealed by its present-day massExpand
Cosmological Constraints on the Properties of Weakly Interacting Massive Particles
Considerations of the age and density of, as well as the evolution of structure in, the universe lead to constraints on the masses and lifetimes of weakly interacting massive particles (WIMPs). TheExpand
The deuterium abundance in the local interstellar medium
As the Galaxy evolves, the abundance of deuterium in the interstellar medium (ISM) decreases from its primordial value: deuterium is ‘astrated’. The deuterium astration factor f D, the ratio of theExpand
On the abundance of primordial helium
We have used recent observations of helium-4, nitrogen and oxygen from some four dozen, low metallicity, extra-galactic HII regions to define mean $N$ versus $O$, $^4He$ versus $N$ and $^4He$ versusExpand
Primordial nucleosynthesis: Theory and observations
We review the cosmology and physics underlying Primordial Nucleosynthesis and survey current observational data in order to compare the predictions of Big Bang Nucleosynthesis with the inferredExpand
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