Abstract

The fusion-evaporation reaction $^{28}\mathrm{Si}+^{40}\mathrm{Ca}$ at 122 MeV beam energy was used to populate excited states in the $N=Z+1$ nucleus $^{63}\mathrm{Ga}$. With the combination of the Gammasphere spectrometer and the Microball CsI(Tl) charged-particle detector array, the level scheme of $^{63}\mathrm{Ga}$ was extended by more than a factor of two in terms of number of $\ensuremath{\gamma}$-ray transitions and excited states, excitation energy $({E}_{x}>30\phantom{\rule{0.16em}{0ex}}\mathrm{MeV})$, and angular momentum $(I>30\phantom{\rule{0.16em}{0ex}}\ensuremath{\hbar})$. Nine regular sequences of states were newly established in the high-spin part of the level scheme. The majority of these rotational band structures could be connected to the previously known part of the level scheme by high-energy $\ensuremath{\gamma}$-ray transitions in the energy range ${E}_{\ensuremath{\gamma}}=4--6\phantom{\rule{0.16em}{0ex}}\mathrm{MeV}$. Low-spin states were assessed by shell-model calculations. The high-spin rotational bands were interpreted and classified by means of cranked Nilsson-Strutinsky calculations.

Highlights

  • The structure of nuclei located in the vicinity of the doubly magic nucleus 56Ni can be expected to be described by the spherical shell model within the full N = 3 f p model space, which comprises the f7/2 orbital below, and the p3/2, f5/2, and p1/2 orbitals above the N = Z = 28 shell gap

  • While this was found to be the case for low-spin states in mass A ≈ 50–60 nuclei [1,2,3,4,5], the situation quickly becomes more complex for slightly heavier N ≈ Z nuclei and likewise as a function of excitation energy and angular momentum

  • Quadrupole deformation was found to increase with the number of particle-hole excitations across the shell gap and the number of particles placed in the g9/2 intruder orbitals

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Summary

Introduction

The structure of nuclei located in the vicinity of the doubly magic nucleus 56Ni can be expected to be described by the spherical shell model within the full N = 3 f p model space, which comprises the f7/2 orbital below, and the p3/2, f5/2, and p1/2 orbitals above the N = Z = 28 shell gap While this was found to be the case for low-spin states in mass A ≈ 50–60 nuclei [1,2,3,4,5], the situation quickly becomes more complex for slightly heavier N ≈ Z nuclei and likewise as a function of excitation energy and angular momentum. The feature of increasing deformation with an increasing number of particles placed in the g9/2 intruder orbitals could be delineated

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Conclusion

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