PArthENoPE reloaded

PArthENoPE reloaded

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PArthENoPE reloaded

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Consiglio, R.; Fernández de Salas, Pablo; Mangano, Gianpiero; Miele, Gennaro; Pastor Carpi, Sergio; Pisanti, Ofelia
Aquest document és un/a article, creat/da en: 2018
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, this http URL 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.

    Consiglio, R. Fernández de Salas, Pablo Mangano, Gianpiero Miele, Gennaro Pastor Carpi, Sergio Pisanti, Ofelia 2018 PArthENoPE reloaded Computer Physics Communications 233 237 242
distribuït sota llicència Creative Commons de Reconeixement-NoComercial 3.0 No adaptada

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