Abstract
The impact of nuclear physics on astrophysical r-process models is discussed, emphasizing the importance of β-decay properties of neutron-rich nuclei. Several r-process motivated β-decay experiments performed at the National Superconducting Cyclotron Laboratory are presented. The experiments include the measurement of β-decay half-lives and neutron emission probabilities of nuclei in regions around 78Ni50; 90Se56; 106Zr66 and 120Rh74, as well as spectroscopic studies of 120Pd74. A summary on the different experimental techniques employed, data analysis, results and impact on model calculations is presented.
Original language | English |
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Journal | Proceedings of Science |
State | Published - 2008 |
Event | 10th Symposium on Nuclei in the Cosmos, NIC 2008 - Mackinac Island, MI, United States Duration: Jul 27 2008 → Aug 1 2008 |