Neutron $3s_{1/2}$ occupation change across the stable tin isotopes investigated using isotopic analysis of proton scattering at 295 MeV
Yoshiko Kanada-En'yo

TL;DR
This study investigates the neutron 3s_{1/2} orbital occupation change across stable tin isotopes using proton scattering at 295 MeV, combining reaction and nuclear structure calculations to analyze isotopic variations.
Contribution
It demonstrates the sensitivity of proton scattering cross section ratios to neutron orbital occupations and compares relativistic and nonrelativistic nuclear density models for isotopic analysis.
Findings
The SKM* density model reproduces experimental cross section ratios better than DD-ME2.
The neutron 3s_{1/2} occupation does not increase rapidly from $^{116}$Sn to $^{122}$Sn.
Results align with direct measurements of neutron occupations in tin isotopes.
Abstract
The isotopic systematics of Sn isotopes in the range A=116--124 were investigated by combining the nuclear structure and reaction calculations for the analysis of Sn(p,p) reactions at 295 MeV. The Sn(p,p) reactions were calculated employing relativistic impulse approximation (RIA) with theoretical densities obtained for the Sn isotopes from relativistic Hartree-Bogoliubov (RHB) calculations with the DD-ME2 interaction and nonrelativistic Skyrme Hartree-Fock-Bogoliubov (SHFB) calculations with the SKM* interaction. Calculation using the DD-ME2 density reproduced the experimental data for Sn(p,p) but overestimated the Sn(p,p) and Sn(p,p) cross sections at backward angles. In the isotopic analysis of the cross section ratio of Sn to Sn, a calculation using the SKM* density reproduced the peak amplitudes of obtained from the…
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Taxonomy
TopicsNuclear physics research studies · Astro and Planetary Science · Nuclear Physics and Applications
