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PArthENoPE Revolutions

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arxiv 2103.05027 v1 pith:6S3BXZIB submitted 2021-03-08 astro-ph.IM

S. Gariazzo , P.F. de Salas , O. Pisanti , R. Consiglio This is my paper · ORCID
classification astro-ph.IM
keywords parthenopecodemainpreviousversionabundancesapartbang
verification ladder T0 review T1 audit T2 compute T3 formal
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This paper presents the main features of a new and updated version of the program PArthENoPE, which the community has been using for many years for computing the abundances of light elements produced during Big Bang Nucleosynthesis. This is the third release of the PArthENoPE code, after the 2008 and the 2018 ones, and will be distributed from the code's website, http://parthenope.na.infn.it. Apart from minor changes, the main improvements in this new version include a revisited implementation of the nuclear rates for the most important reactions of deuterium destruction, H2(p,gamma)He3, H2(d, n)He3 and H2(d, p)H3, and a re-designed GUI, which extends the functionality of the previous one. The new GUI, in particular, supersedes the previous tools for running over grids of parameters with a better management of parallel runs, and it offers a brand-new set of functions for plotting the results.

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Cited by 4 Pith papers

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  3. Impact of non-standard neutrino-electron interactions on Big Bang Nucleosynthesis

    hep-ph 2026-02 conditional novelty 6.0 of 10

    NSI between neutrinos and electrons shift Big Bang Nucleosynthesis yields of helium-4 and deuterium, yielding cosmological constraints that are weaker than but complementary to terrestrial limits.

  4. What could an emerging Big Bang Nucleosynthesis discrepancy be hinting at?

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    A transient expansion-rate boost during deuterium burning can reconcile the measured deuterium abundance with the high baryon density preferred by early dark energy models, without changing helium-4.

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