“…The recently recognized diversity of astrophysical neutron capture processes, including the s-process, the i-process, the r-process, and the n-process, further underscores the need to address the challenge of obtaining neutron capture rates for unstable nuclei. While direct measurements of neutron capture on very short-lived nuclides are presently not feasible, multiple indirect experimental techniques and advances in nuclear-reaction theory make it possible to obtain constraints for important reaction rates (figure 3): β-delayed neutron emission [244,245], the β-Oslo [246,247] and inverse-Oslo [248] methods, transfer reactions [249][250][251], the surrogate reaction method [252][253][254], the Trojan Horse Method [114], and Coulomb breakup [255][256][257] offer pathways to study neutron-capture reactions on short-lived isotopes. In addition, measurements of evaporation spectra at stable-beam facilities [258] provide complementary information for nuclei just off stability, e.g., for those relevant to i-process nucleosynthesis.…”