“…In such conditions, the specific nuclear abundances are expected to depend on the fission properties of many exotic neutron-rich nuclei [16,17,[43][44][45][46][47]. However, these fission properties effectively rely entirely on theory-based predictions, and a great deal of progress has been made to evaluate them, including from systematic, macroscopic-microscopic, and purely microscopic theoretical approaches (see, e.g., [48] and references therein for a recent review; also [16,17,37,[49][50][51][52]). In order to help inform existing and future efforts in the study of nuclear fission, we use our tracing framework to examine the various ways that different fission processes, namely spontaneous fission (sf ), β − -delayed fission (βdf ), and neutron-induced fission ((n, f )), can influence r-process nucleosynthesis in the ejecta of a neutron star merger.…”