Galaxy Rotation Curves as Emergent Non-Equilibrium Structures without Parameter Fitting: Results from the SPARC_Lelli2016c Dataset

This dataset contains the full results associated with the study: "Galaxy Rotation Curves as Emergent Non-Equilibrium Structures without Parameter Fitting: Results from the SPARC_Lelli2016c Dataset" The archive includes RMSE statistics and associated properties for 175 galaxies from the SPARC_Lelli2016c dataset, together with per-galaxy rotation curve comparisons and figures used in the main analysis. All results are generated without per-galaxy parameter fitting. No data filtering or galaxy-specific tuning was applied. The RMSE distribution (Figure 1) is directly computed from the provided dataset (IHG_all_summary.csv) without additional processing beyond standard aggregation. These results demonstrate that the observed galaxy rotation curves arise as emergent structures from a non-equilibrium generative process governed by fixed rules, rather than from parameter fitting or equilibrium assumptions.