Relativity and Cosmology

    

Gravitational Dynamics of Cantor Dust and Self-Interacting Dark Matter

Authors: Ervin Goldfain

We develop a first-principles framework in which self-interacting dark matter (SIDM) emerges as an effective manifestation of primordial Cantor Dust. In this framework, Dark Matter resides on a multifractal support characterized by a scale-dependent Hausdorff dimension D<3. We argue that the phenomenology of SIDM is a memory of primordial Cantor Dust, emerging without conventional particle scattering and cross sections. The mechanism described here reproduces the flat galactic rotation curves, baryonic Tully-Fisher relations, the SIDM transport cross section, explains the core—cusp problem, the evasion of Bullet Cluster bounds and the morphology of the cosmic web.

Comments: 36 Pages.

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[v1] 2026-03-02 13:52:29

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