Beta decay studies of neutron-rich nuclides near N = 32

Details Beta decay studies of neutron-rich nuclides near N = 32 Beta decay studies of neutron-rich nuclides near N = 32

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apro10004m&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

The low-energy levels of ^56Cr_32 and ^54Ti_32 were populated following the β decay of ^56V and ^54Sc, respectively. The parent nuclei were produced following fragmentation of a 140 MeV/nucleon ^86Kr beam, provided by the Coupled Cyclotron Facility at the National Superconducting Cyclotron Laboratory at Michigan State University, in a Be target. The isotopes of interest were separated using the A1900 fragment separator and implanted into a Si microstrip detector. Beta-delayed gamma rays, correlated with fragment implants, were detected using six detectors from the MSU Segmented Ge array. The low-energy structures of ^56Cr and ^54Ti, which support the appearance of a subshell closure at N = 32 for neutron-rich nuclides having Z <= 24, will be discussed.

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