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 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, H-2(p,gamma) He-3, H-2(d, n)He-3 and H-2(d, p)H-3, 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.Program summaryProgram title: PArthENoPE 3.0CPC Library link to program files: https://doi.org/10.17632/wygr7d8yt9.2Developer's repository link: http://parthenope.na.infn.itLicensing provisions: GPLv3Programming language: Fortran 77 and PythonNature of problem: Computation of yields of light elements synthesized in the primordial universeSolution method: Livermore Solver for Ordinary Differential Equations (LSODE) for stiff and nonstiff systems, Python GUI for running and plottingJournal reference of previous version: Comput. Phys. Commun. 233 (2018) 237-242Does the new version supersede the previous version?: YesReasons for the new version: Update of the physics and improvements in the GUISummary of revisions: Update of the physics implemented in the Fortran code and improvements in the GUI functionalities, in particular new plotting functions (C) 2021 Elsevier B.V. All rights reserved.