β-decay studies of r-process nuclei at NSCL

Details β-decay studies of r-process nuclei at NSCL β-decay studies of r-process nuclei at NSCL

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008nupha.805..470p&link_type=abstract

Nuclear Physics A, Volume 805, Issue 1-4, p. 470-477.

Physics

Nuclear Physics

Properties Of Nuclei, Nuclear Energy Levels, Nuclear Structure Models And Methods, Beta Decay, Double Beta Decay, Electron And Muon Capture, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, 59<=A<=89, 90<=A<=149

Scientific paper

Observed neutron-capture elemental abundances in metal-poor stars, along with ongoing analysis of the extremely metal-poor Eu-enriched sub-class provide new guidance for astrophysical models aimed at finding the r-process sites. The present paper emphasizes the importance of nuclear physics parameters entering in these models, particularly β-decay properties of neutron-rich nuclei. In this context, several r-process motivated β-decay experiments performed at the National Superconducting Cyclotron Laboratory (NSCL) are presented, including a summary of results and impact on model calculations.

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