Understanding Excitations in $^{59,61}$Co, $^{59}$Ni

TL;DR

This study investigates high spin states in $^{59}$Co, $^{59}$Ni, and $^{61}$Co using fusion evaporation reactions, expanding known level schemes, confirming and modifying previous data, and highlighting the role of g$_{9/2}$ orbital excitations in nuclear structure.

Contribution

The paper provides new high spin state data, extends level schemes, and demonstrates the significance of g$_{9/2}$ orbital crossing in these nuclei through experimental and shell model analysis.

Findings

Expanded level scheme of $^{59}$Co up to 31/2$^+$ at 11 MeV.

Verified and modified positive parity states in $^{59}$Ni.

Reassigned a band in $^{61}$Co as a magnetic rotation candidate.

Abstract

High spin states in $^{59}$Co ($Z=27$), $^{59}$Ni ($Z=28$) and $^{61}$Co have been populated by the fusion evaporation reactions, $^{48}$Ti($^{14}$C, p2n)$^{59}$Co, $^{48}$Ti($^{14}$C, 3n)$^{59}$Ni, and $^{50}$Ti($^{14}$C, p2n)$^{61}$Co. The 9 MV tandem accelerator at the John D Fox Laboratory, Florida State University (FSU) was used to accelerate the $^{14}$C beam and the de-exciting $\gamma$ rays were detected by the FSU detector array consisting of six High Purity Germanium (HPGe) clover detectors, and three single crystals. Directional correlation of the $\gamma$ rays de-exciting oriented states (DCO ratios) and polarization asymmetry measurements helped to establish spin and parities of the excited states whenever possible. The level scheme of $^{59}$Co has been expanded with the inclusion of positive parity states up to 31/2$^+$ at around 11 MeV. The $^{59}$Ni positive parity states known from previous study were verified with modifications to some of the spins and parities. On the other hand, the negative parity states were extended to 31/2 at an excitation energy of 12 MeV. No new transition was observed for $^{61}$Co, but one of the major bands has been reassigned as consisting of positive parity states by reason of this study which is a candidate for magnetic rotation band. Cross shell excitations were observed in the three nuclei studied and the prominent role of excitation to g$_{9/2}$ orbital crossing the $N=40$ shell gap was established in relation to collective excitation in these nuclei by comparison with large-scale shell model calculations.