Shell Model Calculations of Nuclear Properties in (91,93Sr) Strontium Isotopes Using NuShellX@MSU Code

Authors

  • F. H. Obeed Department of Physics, Faculty of Education for Girls, University of Kufa, Najaf, Iraq
  • A. K. Hasan College of Health and Medical Technology, University of Alkafeel, Iraq

Keywords:

Energy spectra, Transition strengths, Density distributions

Abstract

Abstract: The nuclear shell model has been applied to calculate various nuclear properties of the 91,93Sr isotopes, including spins and parities, energy spectra, reduced electromagnetic transition possibilities (electric quadrupole and magnetic dipole), magnetic dipole moments, nuclear charge distributions, and mass density as functions of the radial distance from the nucleus center (r). In this study, the NuShellX@MSU code was employed using Gloeckner-Bare G-matrix interaction, within the Gloeckner model space of the orbits (2p1/2,1g9/2) and (3s1/2,2d5/2) for protons and neutrons, respectively. The results showed good agreement with the available experimental data (spins and parities of energy spectra) and a confirmation of most levels. Theoretically, new values have been expected for the most nuclear properties, including spin, parities, energy spectra, transition strengths, electric quadrupole, dipole magnetic moments, the nuclear charge, and mass density distributions. Previously, these accounts had not been determined empirically.

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Published

2025-08-23

How to Cite

Obeed, F. H., & Hasan, A. K. (2025). Shell Model Calculations of Nuclear Properties in (91,93Sr) Strontium Isotopes Using NuShellX@MSU Code. Jordan Journal of Physics, 18(2), 131–140. Retrieved from https://jjp.yu.edu.jo/index.php/jjp/article/view/1126