AlterBBN v2: A public code for calculating Big-Bang nucleosynthesis constraints in alternative cosmologies

被引:60
作者
Arbey, A. [1 ,2 ]
Auffinger, J. [1 ,3 ]
Hickerson, K. P. [4 ]
Jenssen, E. S. [5 ]
机构
[1] Univ Lyon, Univ Claude Bernard Lyon 1, CNRS IN2P3, IP21 Lyon,UMR 5822, F-69622 Villeurbanne, France
[2] CERN, Theoret Phys Dept, CH-1211 Geneva 23, Switzerland
[3] Ecole Normale Super Lyon, F-69342 Lyon, France
[4] CALTECH, WK Kellogg Radiat Lab, Pasadena, CA 91125 USA
[5] Univ Oslo, Inst Theoret Astrophys, Boks 1072 Blindern, N-0316 Oslo, Norway
关键词
Big-Bang nucleosynthesis; Early universe; Alternative cosmologies; WIMPs; FLAVOR PHYSICS OBSERVABLES; RELIC DENSITY; ELEMENTS; PROGRAM; ABUNDANCES;
D O I
10.1016/j.cpc.2019.106982
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
We present the version 2 of AlterBBN, an open public code for the calculation of the abundance of the elements from Big-Bang nucleosynthesis. It does not rely on any closed external library or program, aims at being user-friendly and allowing easy modifications, and provides a fast and reliable calculation of the Big-Bang nucleosynthesis constraints in the standard and alternative cosmologies. Program summary Program Title: AlterBBN Program Files doi: http://dx.doi.org/10.17632/k7j3b9zyvf.1 Licensing provisions: GNU General Public License 3 Programming language: C Journal Reference of previous version: Comput. Phys. Commun. 183 (2012) 1822 Does the new version supersede the previous version: Yes Reasons for new version: AlterBBN v2 is a major update of AlterBBN, with an expanded nuclear network, new integration methods and new cosmological scenarios. Summary of revisions: Implementation of several numerical integration methods Automatic error and correlation calculation Extended nuclear network Cosmological scenarios with decaying scalar field or reheating Scenarios with WIMPs Interface with the JINA REACLIB nuclear database Parallelization using OpenMP Nature of problem: Calculation of the abundance of the elements generated during Big-Bang Nucleosynthesis (BBN). Solution method: AlterBBN computes the abundance of the elements by solving the system of cosmological and Boltzmann equations for each of the isotopes. It features different numerical methods adapted to stiff problems. The cosmological equations can be modified in order to test the cosmological assumptions and test alternative scenarios. Unusual features: AlterBBN has been parallelized and use the OpenMP library. (C) 2019 Elsevier B.V. All rights reserved.
引用
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页数:21
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