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

J. Pereira, A. Aprahamian, O. Arndt, A. Becerril, T. Elliot, A. Estrade, D. Galaviz, S. Hennrich, R. Kessler, K. L. Kratz, G. Lorusso, P. F. Mantica, M. Matos, F. Montes, P. Santi, B. Pfeiffer, M. Quinn, H. Schatz, F. Schertz, L. SchnorrenbergerE. Smith, B. E. Tomlin, W. Walters, A. Wöhr

Research output: Contribution to journalConference articlepeer-review

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 languageEnglish
JournalProceedings of Science
StatePublished - 2008
Event10th Symposium on Nuclei in the Cosmos, NIC 2008 - Mackinac Island, MI, United States
Duration: Jul 27 2008Aug 1 2008

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