PArthENoPE Revolutions
arXiv:2103.05027 · doi:10.1016/j.cpc.2021.108205
Abstract
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.
arXiv comment28 pages, 7 figures
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- Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB
- Constraining Feeble Neutrino Interactions with Ultralight Dark Matter
- Bayesian Estimation of the D(p,)He Thermonuclear Reaction Rate
- Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
- Was Entropy Conserved between BBN and Recombination?
- Big bang nucleosynthesis and early dark energy in light of the EMPRESS results and the tension
- Updated cosmological constraints on Macroscopic Dark Matter
- Beyond Fisher Forecasting for Cosmology