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The impact of nuclear physics on astrophysical r-process models is discussed,emphasizing the importance of beta-decay properties of neutron-rich nuclei.Several r-process motivated beta-decay experiments performed at the NationalSuperconducting Cyclotron Laboratory are presented. The experiments include themeasurement of beta-decay half-lives and neutron emission probabilities ofnuclei in regions around Ni-78; Se-90; Zr-106 and Rh-120, as well asspectroscopic studies of Pd-120. A summary on the different experimentaltechniques employed, data analysis, results and impact on model calculations ispresented.

Beta decay studies of r-process nuclei at the National Superconducting Cyclotron Laboratory