## 5 Conclusions
The strong consistency observed between the angular differential scattering cross sections simulated using the TALYS 1.96 nuclear reaction code and the EXFOR experimental data--based on nucleon densities calculated via the SHF-WS model and the corresponding SF interaction potentials--provides encouraging evidence for the accuracy and applicability of the theoretical model as a complementary approach. In particular, the distinct structures observed at approximately 50\({}^{\circ}\) in the 4.87 MeV and 6 MeV energy regions of the \({}^{182}\)W(n,el) and \({}^{184}\)W(n,el) reactions are not only clearly present in the experimental data but are also accurately reproduced using the SHF-WS + SF + TALYS 1.96 approach. These features, which are not well captured by traditional OMP (e.g., Koning and Delaroche), indicate that this simulation-based methodology can potentially resolve finer details in certain cases where conventional models show limitations. This success contributes a new dimension to our understanding of nuclear structure in several respects:  
Since the SHF model is based on microscopic principles, it describes the distribution of nucleons within the nucleus according to fundamental interactions, rather than relying on parameterized fits to experimental data. As a result, structural properties of neutron-rich nuclei can be represented more accurately. This enables reliable predictions of nucleon density distributions, especially for exotic or unstable isotopes, where experimental data are limited or inaccessible. The SF approach derives the Nn interaction potential by integrating the NN interaction over the target nucleus density, offering a more physically grounded method compared to classical OMP parameterizations. Through this technique, the diffraction-like structure of the angular distribution--reflecting changes in the scattering centers with energy--is naturally reproduced. The graphical analysis reveals several new insights:
* Proliferation of energy-dependent diffraction structures The increasing number of peaks and valleys observed at higher energies can be attributed to the shortening of the wavelength. This suggests that scattering occurs not over the entire nucleus but rather on individual nucleons, thereby enhancing the visibility of nuclear shell effects. * Discrepancies in backward scattering Although the model generally preserves the overall shape of the distribution, it fails to fully reproduce certain peak structures around 150\({}^{\circ}\). This indicates that there is still room for improvement in the model, particularly in better accounting for spin-orbit effects and many-body correlations. Detailed modeling of neutron elastic scattering reactions enables more precise results in practical applications such as reactor physics and radiation shielding design. Moreover, this modeling approach allows for the generation of high-accuracy nuclear reaction data for isotopes lacking experimental measurements, thereby contributing to nuclear data libraries such as ENDF and TENDL. This study demonstrates that, beyond the conventional OM, constructing interaction potentials based on microscopically derived nuclear densities can achieve better agreement with experimental data and provide deeper insights into nuclear structure. In this respect,it represents a significant step toward theoretical data generation, particularly for exotic or experimentally inaccessible systems. Based on the graphical analysis, the following general conclusions can be drawn:  
Advantages of the model:  
The angular resolution is particularly high at medium to high energies. The positions and numbers of the diffraction-like structures observed experimentally are largely well reproduced. Limitations and areas for improvement:  
Some minima and maxima at backward scattering angles have been overlooked. This may be due to the model's current exclusion of additional effects such as spin-orbit forces or channel coupling.