PArthENoPE Revolutions

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 an...

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Veröffentlicht in:arXiv.org 2021-03
Hauptverfasser: Gariazzo, S, de Salas, P F, Pisanti, O, Consiglio, R
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description 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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subjects Big bang cosmology
Deuterium
Graphical user interface
Light elements
Nuclear fusion
Nuclei (nuclear physics)
Physics - Instrumentation and Methods for Astrophysics
Websites
title PArthENoPE Revolutions
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