PArthENoPE reloaded
R. Consiglio, P.F. de Salas, G. Mangano, G. Miele, S. Pastor, and O., Pisanti
TL;DR
This paper introduces PArthENoPE 2.0, an updated version of a code for calculating primordial light element abundances, featuring improved computational libraries and a user-friendly GUI, enhancing accessibility and usability.
Contribution
The paper presents significant updates to PArthENoPE, including replacing proprietary routines with open-source libraries and adding a GUI for easier use and parameter exploration.
Findings
Validated new version against previous results
Demonstrated ease of use with GUI
Provided results for minimal BBN scenario
Abstract
We describe the main features of a new and updated version of the program PArthENoPE, which computes the abundances of light elements produced during Big Bang Nucleosynthesis. As the previous first release in 2008, the new one, PArthENoPE 2.0, will be soon publicly available and distributed from the code site, http://parthenope.na.infn.it. Apart from minor changes, which will be also detailed, the main improvements are as follows. The powerful, but not freely accessible, NAG routines have been substituted by ODEPACK libraries, without any significant loss in precision. Moreover, we have developed a Graphical User Interface (GUI) which allows a friendly use of the code and a simpler implementation of running for grids of input parameters. Finally, we report the results of PArthENoPE 2.0 for a minimal BBN scenario with free radiation energy density.
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