Sensitivity of r-nuclide distributions to the choice of nuclear mass model
V. Negrebetskiy*, E. Vladimirova, M. Simonov, K. Stopani and T. Tretyakova
Pre-published on:
March 09, 2022
Published on:
May 24, 2022
Abstract
Theoretical estimates of the cross sections and rates of neutron capture reactions in the astrophysical p-process are obtained using the masses of unknown nuclei predicted in such approaches as FRDM, HFB and WS+RBF. We also used the mass values obtained by us in the phenomenological approach using local mass relations. Variations of predicted r-process yields, caused by nuclear models uncertainties, were studied.
DOI: https://doi.org/10.22323/1.380.0333
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating
very compact bibliographies which can be beneficial to authors and
readers, and in "proceeding" format
which is more detailed and complete.