6533b85afe1ef96bd12b9891
RESEARCH PRODUCT
PArthENoPE reloaded
Gianpiero ManganoP. F. De SalasOfelia PisantiR. ConsiglioGennaro MieleSergio Pastorsubject
Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesGeneral Physics and AstronomyAstrophysicscomputer.software_genre01 natural sciencesPartícules (Física nuclear)Physics and Astronomy (all)High Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesCode (cryptography)010306 general physicsGraphical user interfaceParthenopePhysicsCosmologiaPrimordial nucleosynthesi010308 nuclear & particles physicsProgramming languagebusiness.industryCosmologyNeutrino physicHigh Energy Physics - PhenomenologyHardware and ArchitecturebusinesscomputerAstrophysics - Cosmology and Nongalactic Astrophysicsdescription
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.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2018-01-01 |