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The recent observation of neutron stars merger by the Laser InterferometerGravitational-Wave Observatory (LIGO) collaboration and the measurements of theevent's electromagnetic spectrum as a function of time for differentwavelengths have altered profoundly our understanding of the r-process site aswell as considerably energized nuclear astrophysics research efforts. R-processabundances are a key element in r-process simulations, as a successfulcalculation must account for these abundances in the final debris of a stellarcataclysmic event. In this article, mankind's complete knowledge of neutroncross sections obtained over the last 80 years, as encapsulated in the latestrelease of the Evaluated Nuclear Data File (ENDF/B) library, is used to obtainsolar system r-process abundances in a comprehensive data approach. ENDF/Bcross sections have been successfully used for decades in nuclear power anddefense applications and are now used to obtain r-process abundances in a fullytraceable and documented way. This article r-process abundances providecomplementary insights on the astrophysical events, overall quality of neutroncapture data in the astrophysical region of temperatures, and demonstrateissues with the s-process contribution subtraction procedure.

Capitalizing on Nuclear Data Libraries' Comprehensiveness to Obtain Solar System r-process Abundances