\begin{document}$ ^{124} $\end{document}Sn from the \begin{document}$ ^{12} $\end{document}C + \begin{document}$ ^{124} $\end{document}Sn elastic scattering angular distribution, obtaining values of \begin{document}$ 0.168_{\text{−}0.019}^{+0.025} $\end{document} fm (SLy4) and \begin{document}$ 0.177 \pm 0.022 $\end{document} fm (SLy7). These results are consistent with measurements from various other methods. Furthermore, through correlation analysis between the neutron skin thickness and nuclear symmetry energy slope parameter L, we determined the symmetry energy slope coefficients to be \begin{document}$ L = 39.0_{\text{−}16.5}^{+20.8} $\end{document} MeV (SLy4) and \begin{document}$L = 46.1 \pm 18.7$\end{document} MeV (SLy7) based on the scattering data. These findings validate existing theoretical models and provide valuable insights for further studies on neutron stars and nuclear matter properties."> Extracting the neutron skin thickness of <sup>124</sup>Sn from the <sup>12</sup>C + <sup>124</sup>Sn elastic scattering angular distribution -
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