Primordial Light Element Abundances
Paolo Molaro

TL;DR
This paper reviews primordial light element abundances, their measurement, and implications for cosmology, highlighting recent revisions and ongoing puzzles in lithium abundance discrepancies.
Contribution
It provides an updated synthesis of observational data and theoretical models, emphasizing the impact of new atomic physics and systematics on primordial abundance estimates.
Findings
Revised helium abundance reduces tension with WMAP data.
D/H measurements align with WMAP predictions despite scatter.
Lithium abundance remains significantly lower than theoretical expectations.
Abstract
After few minutes the Universe evolved through conditions of temperature and density which permitted the first synthesis of astrophysically interesting abundances of D, 3He, 4He and 7Li. The relic abundances are sensitive probes of the nucleon density and so are the CMB acoustic oscillations, somewhat 400000 years later, which allow a stringent cross check. The CMB high precision estimate of the baryon density by WMAP is currently used as input parameter for standard big bang nucleosynthesis (SBBN) to interpret primordial bundances rather then being directly derived from the observations of light elements as was common use before. New atomic physics and identification of systematics lead to an upwards revision of the 4He primordial abundance at Yp=0.2477 +/- 0.0029 (Peimbert et al 2007) removing a major source of tension between SBBN and WMAP. The D/H as measured in QSO high redshift…
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Taxonomy
TopicsAstro and Planetary Science · Nuclear physics research studies
