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A geometric resolution limit from vacuum entanglement: Topological Structure and Particle-Wave Asymmetry

Isbelia Martin

hep-tharXiv:2608.27640

Abstract

We establish that the entanglement entropy of the electromagnetic vacuum, when regulated by weak spacetime curvature, imposes a fundamental lower bound on the radial resolution available to quantum excitations. Starting from the area law of vacuum entanglement, we demonstrate how linearized gravity introduces a natural ultraviolet regulator via the perturbative Green's function. An exact geometric projection from tangential to radial resolution yields a minimal radial scale Δr rs2/R, where rs is the Schwarzschild radius of the enclosing body and R is the boundary radius. We analyze how particle propagation regimes depend on the relation between the Compton wavelength λC and Δr, showing that consistency λC Δr defines a global, environment-dependent mass scale mgeo R/(c rs2). Measured particle masses satisfy m = αmgeo, where α is a dimensionless factor encoding the vacuum's informational structure. In this extended version, we show that the vacuum resolution limit affects massive and massless excitations asymmetrically. For massive particles with λC Δr, the vacuum appears smooth and transparent, yielding classical geodesic motion. For photons with λ Δr, the vacuum cannot sustain phase coherence, leading to decoherence or dispersion. We argue that this asymmetry follows naturally if λC is interpreted not as a wave scale but as the core size of a topologically stable excitation (knot, vortex, or soliton) in the quantum vacuum field. This framework reframes mass as a probe of vacuum-imposed resolution limits set by global geometry and entanglement, offering a structural perspective on the hierarchy problem and yielding distinct, falsifiable predictions for high-energy propagation.

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