Study of high spin states in <sup>62</sup>Ni with GRETINA at ANL
ORAL
Abstract
High spin states in 62Ni were populated in a fusion evaporation reaction with a 190 MeV 48Ca beam on an isotopically enriched 18O target at Argonne National Laboratory. The de-exciting gamma rays were detected by GRETINA (Gamma-Ray Energy Tracking In-beam Nuclear Array), which consisted at that time of 12 modules positioned to cover polar angles between 700 and 1700. The spins and parities of excited levels were established using angular distribution and polarization asymmetry measurements. This allowed us to identify excited states formed by nucleon excitations within the fp shell and those involving neutron excitations into the g9/2 orbital.
Two additional rotational bands have been added to the two existing rotational bands. The excitations within the fp shell and those with one neutron excited into the g9/2 orbital were found to be consistent with large-scale shell model calculations. Deviations were, however, observed between the experimental results and the shell model calculations for high spin states, suggesting the importance of the two neutron excitations into the g9/2 orbital not captured by the shell model calculations. These experimental results emphasized the need for refining the calculations to align with the suggested 2p-2h configurations of the states. Calculations using the Generator Coordinate Method were found to be more consistent with the 2p-2h excitations.
This work is supported by US NSF under Grant # PHY 2412808 (FSU) and the UD Department of Energy under Grant # DE-FG02-94ER40848 (UML) and DE-AC52-07NA27344 (LLNL)
Two additional rotational bands have been added to the two existing rotational bands. The excitations within the fp shell and those with one neutron excited into the g9/2 orbital were found to be consistent with large-scale shell model calculations. Deviations were, however, observed between the experimental results and the shell model calculations for high spin states, suggesting the importance of the two neutron excitations into the g9/2 orbital not captured by the shell model calculations. These experimental results emphasized the need for refining the calculations to align with the suggested 2p-2h configurations of the states. Calculations using the Generator Coordinate Method were found to be more consistent with the 2p-2h excitations.
This work is supported by US NSF under Grant # PHY 2412808 (FSU) and the UD Department of Energy under Grant # DE-FG02-94ER40848 (UML) and DE-AC52-07NA27344 (LLNL)
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Presenters
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Vandana Tripathi
Florida State University
Authors
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Vandana Tripathi
Florida State University
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Samuel Oluwamayowa Ajayi
Florida State University
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Peter C Bender
University of Massachusetts Lowell
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Brenden Longfellow
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Soumik Bhattacharya
Florida State University