Constrained SO(3,3) Spacetime: Part IV. Kinematic Phase-Anchoring and the Asymptotic Classical Limit

Abstract

Operating under the theoretical assumption that a topological constraint field provides an effective kinematic barrier against negative-norm ghost states in an SO(3,3) spacetime, this paper explores the geometric relationship between mass, relativistic momentum, and transverse-time quantum tunneling. While previous work hypothesized that microscopic particles might temporarily leak into uncompactified temporal dimensions to form quantum superpositions, we propose that this vulnerability might be asymptotically suppressed as a system scales in mass or velocity. Specifically, we suggest that increasing rest mass and kinetic energy could dynamically amplify a macroscopic "Phase-Anchor" effect, potentially restricting the temporal vectors of massive or highly energetic states to align strictly with the 1D Meta-Time axis. By exploring the modified energy-momentum dispersion relation, we hypothesize that this amplified geometric resistance could drive the probability of transverse-time tunneling toward zero. This paper serves as a theoretical proposal, suggesting that the transition from quantum fuzziness to classical determinism might emerge as a direct geometric consequence of topological inertia, thereby outlining a conceptual boundary condition for future rigorous algebraic investigations.