The Nuclear R package provides a set of functions to simulate and estimate non-resonant astrophysical S-factors and thermonuclear reaction rates, based on measured nuclear cross sections. The following reactions are currently included: d(p,γ)3He, d(d,n)3He, d(d,p)3H, 3H(d,n)4He, 3He(3He,2p)4He, 3He(α,γ)7Be, 3He(d,p)4He, 7Be(n,p)7Li.
d(p,γ)3He
d(d,n)3He
d(d,p)3H
3H(d,n)4He
{r,results='hide',message=FALSE, cache=FALSE}
require(devtools)
devtools::install_github("rafaelsdesouza/nuclear")
de Souza, Rafael S.; Iliadis, Christian; Coc, Alain, Astrophysical S-factors, Thermonuclear Rates, and Electron Screening Potential for the 3He(d,p)4He Big Bang Reaction via a Hierarchical Bayesian Model, Astrophys. J. 872, 1 (2019).
de Souza, Rafael S.; Boston, S. Reece; Coc, Alain; Iliadis, Christian, Thermonuclear fusion rates for tritium + deuterium using Bayesian methods, Physical Review C 99, 1, 014619 (2019).
C. Iliadis, K.S. Anderson, A. Coc, F.X. Timmes, and S. Starrfield, Bayesian Estimation of Thermonuclear Reaction Rates, Astrophys. J. 831, 107 (2016).
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