Numerical analysis explores baryonic matter dynamics and galaxy rotation curves, indicating potential for educational use.
This repository contains the full Dynamic Local Mass Clustering (DLMC) analysis, including numerical notebooks, figures, and scripts. The study explores baryonic matter dynamics, spatial decoupling in galaxy rotation curves, and visualization of key outputs. The notebooks are ready for reproducibility and educational purposes, with code and markdown organized for clarity.
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mounir djebassi (2026) studied this question.
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