Artificial Intelligence Supported Shell-Model Calculations for Light Sn Isotopes
Serkan Akkoyun, Abderrahmane Yakhelef

TL;DR
This paper uses artificial neural networks to estimate the spectrum of the $^{101}Sn$ isotope, improving shell model calculations for light Sn isotopes and achieving better agreement with experimental data.
Contribution
It introduces an AI-based method to determine neutron single-particle energies, enhancing nuclear structure modeling for Sn isotopes.
Findings
Neural network estimates of $^{101}Sn$ spectrum align well with experimental data.
Shell model calculations with new SPEs show improved accuracy.
The approach offers a new way to obtain missing experimental nuclear data.
Abstract
The region around the doubly magic nuclide is very interesting for nuclear physics studies in terms of structure, reaction and nuclear astrophysics. The main ingredients in nuclear structure studies using the shell model are the single-particle energies and the two-body matrix elements. To obtain the former, experimental data of isotope spectrum are necessary. Since there is not enough experimental data, different approaches are used in the literature to obtain single-particle energies. In sn100pn interaction, the hole excitation spectrum was used in to determine neutron single-particle energies. The other approach is the use of the lightest isotope, , which figures the model space orbitals. In this study, we estimated the spectrum of the isotope by artificial neural network method in order to obtain neutron single-particle energies.…
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