README.md

Nuclear

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

Install Nuclear R package

{r,results='hide',message=FALSE, cache=FALSE} require(devtools) devtools::install_github("rafaelsdesouza/nuclear")

References

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).



RafaelSdeSouza/nuclear documentation built on Aug. 11, 2019, 12:31 a.m.