The_Hubble_Tension_as_a_Macroscopic_Topological_Residual_in_Conformal_Arc_Geometry

Arcman

The Hubble Tension as a Macroscopic Topological Residual

In Conformal Arc Geometry

(Eprint DOI: 10.5281/zenodo.19045059)

In standard cosmology, the Hubble constant H0 parametrizes the kinematic expansion rate of the spacetime metric. However, early-universe (CMB) and late-universe (supernovae) measurements exhibit a persistent discrepancy known as the Hubble Tension. In this Letter, we demonstrate that cosmic expansion is not the stretching of a fundamental metric. Instead, human observation is bounded by the precipitation of natural energy into measurable energy, whose geometric mapping is exactly the Arc Spin. We show that early and late cosmological measurements probe twofundamentally different geometric ground states of Arc Spins: the sequential interaction (wavelike kinematics) and the simultaneous interaction (mass-like kinematics). The transition between these states necessitates a spontaneous topological doubling. Consequently, the Hubble Tension is not a measurement crisis, but an exact macroscopic topological residual—a conformal phase shift structurally required by the Arc Cluster Structure of the universe.


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