The Dark Metapol Framework; A Dynamical Conceptual Model of Protogalactic Angular Momentum, External Dark Matter Infall, Halo Evolution, and Central Density Changes
The Dark Metapol Framework is an exploratory dynamical model based on the standard dark matter cosmological framework, examining the possible relationships between angular momentum formation in protogalaxies, dark matter infall, galactic halo evolution, and changes in central density. The framework considers how primordial rotational conditions may influence the subsequent dynamical development of galaxies, while external dark matter infall contributes to the evolution of galactic halos. It explores the possibility that differences in mass, gravitational interaction, and angular momentum distribution may produce different dynamical responses, influencing the distribution of dark matter between the outer halo and central regions.Particular attention is given to the relationship between dark matter accumulation, central density evolution, and the emergence of approximately flat galactic density profiles. Rather than assuming that central dark matter accumulation necessarily leads to a persistent density cusp, the framework considers how competing dynamical processes may contribute to changes in the central density structure over time.The Dark Metapol Framework is proposed as a conceptual and theoretical model for organizing these interconnected dynamical processes. It does not claim to replace established cosmological models or demonstrate a new dark matter mechanism. Its purpose is to provide an exploratory perspective that may help formulate questions about galaxy formation, angular momentum evolution, dark matter distribution, and the development of galactic core structures.Further mathematical development, numerical simulations, and comparison with astronomical observations are required to assess its physical consistency and predictive potential.
Authors
- Sungmin Lee (ORCID: https://orcid.org/0009-0007-3779-5555)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-11-05
- DOI
- https://doi.org/10.5281/zenodo.23983587
- Primary Topic
- Galaxies: Formation, Evolution, Phenomena
- Type
- preprint