The Structural Interpretation of Dark Matter

This paper develops a structural interpretation of dark matter that reframes the phenomenon as a binding requirement rather than an additional material component of the universe. By stripping the system to its structural essentials and reconstructing the phenomenon from first principles, the paper shows that dark matter can be understood as the binding remainder that appears when visible matter cannot satisfy the coherence demands of astrophysical systems.The argument proceeds in three stages: identifying the structural signature of the phenomenon, reducing it to its stripped structural form, and reconstructing its observational expression without invoking new particles or modifications to gravity. The result is a conceptually economical framework that preserves all empirical successes of the standard model while offering a clearer account of why dark‑matter behavior emerges across galaxies, clusters, and the cosmic web.This interpretation does not replace existing cosmological models; instead, it provides a complementary structural lens that clarifies the role dark matter plays in stabilizing large‑scale systems. The paper concludes by outlining observational implications, theoretical consequences, and avenues for future work grounded in this binding‑based perspective.