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Special Issues
Energy Levels Calculations of 29S, 30S and 31S Isotopes
American Journal of Modern Physics
Volume 4, Issue 3-1, May 2015, Pages: 5-9
Received: Jan. 18, 2015; Accepted: Jan. 28, 2015; Published: Mar. 2, 2015
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Saeed Mohammadi, Department of Physics, Payame Noor University, Tehran, Iran
Sara Sirjani, Department of Physics, Payame Noor University, Tehran, Iran
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In this article by using OXBASH shell model code the energy levels of Sulfur isotopes 29S – 31S are calculated. This code which is based on one of the most applicable nuclear models, deals with evaluating energy levels. Applying the program for each isotope using the defined codes, introduces several files which each file contains a set of data. Meanwhile, the ground state of excitation energy evaluated by OXBASH code together with energy levels and also probable places for nucleons placements in each energy level. Programs will be reliable only when results meet experimental procedures. A compilation of SD-shell energy levels calculated with the USD Hamiltonian and has been published around 1988. A comparison had been made between our results and the available experimental data to test theoretical shell model description of nuclear structure in Sulfur isotopes. The calculated energy spectrum is in good agreement with the available experimental data.
Sulfur Isotopes, OXBASH Code, Shell Model Structure, USD Interaction
To cite this article
Saeed Mohammadi, Sara Sirjani, Energy Levels Calculations of 29S, 30S and 31S Isotopes, American Journal of Modern Physics. Special Issue: Many Particle Simulations. Vol. 4, No. 3-1, 2015, pp. 5-9. doi: 10.11648/j.ajmp.s.2015040301.12
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