Maintainer and Lead Developer since June 2025
AZURE2
A widely used R-matrix code for nuclear astrophysics
AZURE2 fits a multi-level, multi-channel R-matrix model to the measured cross sections, angular distributions and scattering data of every reaction that shares a compound nucleus, and extrapolates the result to the energies at which stars burn. From the fitted cross section it also computes the reaction rate.
It is used for nuclear astrophysics, for nuclear-data evaluation at the IAEA and for ion-beam analysis of materials. I have maintained it and led its development since June 2025: analytic gradients for fits and Markov chain Monte Carlo, a reaction-rate integrator, polarization observables, identical-particle scattering, the graphical interface and the documentation.
What it is for
- —Fitting R-matrix parameters to cross-section data from several reaction channels at once
- —Extrapolating an S-factor below the lowest measured energy
- —Reaction rates and their uncertainties
- —Separating a measured cross section into its resonant and non-resonant parts
How to cite
R. E. Azuma et al., AZURE: An R-matrix code for nuclear astrophysics, Phys. Rev. C 81, 045805 (2010). doi:10.1103/PhysRevC.81.045805
The evaluations on this site run AZURE2 itself, on published analyses and on work not yet published (each page says which); the input files can be downloaded and run locally.