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Review of Big Bang Nucleosynthesis and Primordial Abundances

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arxiv astro-ph/0001318 v1 pith:AXLJWCFL submitted 2000-01-18 astro-ph

David Tytler , John M. O'Meara , Nao Suzuki , Dan Lubin (UC San Diego) This is my paper · ORCID
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keywords abundancesbangnucleinucleosynthesisprimordialreviewabridgedconcentrates
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Big Bang Nucleosynthesis (BBN) is the synthesis of the light nuclei, Deuterium, He3, He4 and Li7, during the first few minutes of the universe. This review concentrates on recent improvements in the measurement of the primordial (after BBN, and prior to modification) abundances of these nuclei. We mention improvement in the standard theory, and the non-standard extensions which are limited by the data. (abridged)

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Mapping the Universe as a Bianchi I cosmology with Gaia data

    astro-ph.CO 2026-05 unverdicted novelty 5.0 of 10

    Gaia quasar proper motions show a significant quadrupole signal matching an axisymmetric Bianchi I anisotropy model, but the amplitude does not increase with redshift as the model requires and the inferred local shear...

  2. Updated BBN Bounds on Hadronic Injection in the Early Universe: The Gravitino Problem

    hep-ph 2025-01 conditional novelty 3.0 of 10

    With current light-element abundances, hadronic decays of long-lived particles are excluded above a yield curve in lifetime, and for gravitinos this translates into reheating temperature upper limits as low as 5×10^5 GeV.

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