PArthENoPE reloaded
NAGIOS: RODERIC FUNCIONANDO

PArthENoPE reloaded

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PArthENoPE reloaded

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dc.contributor.author Consiglio, R.
dc.contributor.author Fernández de Salas, Pablo
dc.contributor.author Mangano, Gianpiero
dc.contributor.author Miele, Gennaro
dc.contributor.author Pastor Carpi, Sergio
dc.contributor.author Pisanti, Ofelia
dc.date.accessioned 2018-10-05T13:18:03Z
dc.date.available 2020-07-30T04:45:05Z
dc.date.issued 2018
dc.identifier.uri http://hdl.handle.net/10550/67722
dc.description.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, 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.
dc.language.iso eng
dc.relation.ispartof Computer Physics Communications, 2018, vol. 233, p. 237-242
dc.rights.uri info:eu-repo/semantics/openAccess
dc.source Consiglio, R. Fernández de Salas, Pablo Mangano, Gianpiero Miele, Gennaro Pastor Carpi, Sergio Pisanti, Ofelia 2018 PArthENoPE reloaded Computer Physics Communications 233 237 242
dc.subject Cosmologia
dc.subject Partícules (Física nuclear)
dc.title PArthENoPE reloaded
dc.type info:eu-repo/semantics/article
dc.date.updated 2018-10-05T13:18:03Z
dc.identifier.doi https://doi.org/10.1016/j.cpc.2018.06.022
dc.identifier.idgrec 127538
dc.embargo.terms 2 years

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