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Nucleosynthesis Without a Computer

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arxiv astro-ph/0303073 v1 pith:DETQHGJ5 submitted 2003-03-04 astro-ph

V. Mukhanov This is my paper · ORCID
classification astro-ph
keywords elementslightnucleosynthesisabundancesanalyticallybe-7big-bangcompletely
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I derive completely analytically the time evolution and final abundances of the light elements (up to Be-7) formed in the big-bang nucleosynthesis.This highlights an interesting physics taking place during the formation of light elements in the early universe.

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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. The Bearable Inhomogeneity of the Baryon Asymmetry

    hep-ph 2025-05 conditional novelty 6.0 of 10

    BBN deuterium abundances exclude baryon-to-photon inhomogeneities above roughly 26-28% RMS, probing physics at temperatures up to a few TeV.

  2. Baryon asymmetry from higher-order matter contributions in gravity

    gr-qc 2025-04 conditional novelty 6.0 of 10

    A T^2-dependent coupling between the derivative of T_mu nu T^mu nu and the baryon current can generate the observed baryon asymmetry in GR and f(R,T^2) gravity, at the cost of fitted parameters.

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