$^{35,37,39}$S isotopes in $sd-pf$ space : Shell-model interpretation
Archana Saxena, P. C. Srivastava, Jorge G. Hirsch, V. K. B. Kota and, M. J. Ermamatov

TL;DR
This paper uses shell model calculations with SDPF-U and SDPFMW interactions to analyze the structure of sulfur isotopes $^{35,37,39}$S, comparing results with experimental data to understand their nuclear configurations.
Contribution
It provides a comprehensive shell model interpretation of sulfur isotopes in the $sd$-$pf$ space, highlighting the role of in-shell and inter-shell excitations with different interactions.
Findings
Good agreement of calculated energy levels with experimental data
Natural parity states described by in-shell mixing
Unnatural parity states require neutron excitations across shells
Abstract
The structure of S isotopes is described by performing comprehensive shell model calculations with SDPF-U and SDPFMW interactions. Protons and neutrons are restricted to the -shell for , neutrons start to fill the -shell for . Natural parity states are described by only in-shell mixing, unnatural parity states with 1p-1h inter-shell neutron excitations. With SDPF-U interaction, reported are the results for natural parity states only because this interaction is not suitable for cross shell excitations. Calculated energy levels, electromagnetic properties and spectroscopic factors are in good agreement with the recently available experimental data.
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