ETT Hypothesis 3 — Part B: A Density-Dependent Breakdown of Higgs Mass Licensing and therefore the de-emergence of Gravity, Weight, Inertia, and Time in the ultra-dense regime

J. E. Holland (2025)
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This paper presents Part B of the Expanse Tension Theory (ETT) Hypothesis 3 framework, extending the unified Holland–Higgs scalar field model developed in Part A into the ultra-dense regimes characteristic of neutron-star interiors and gravitational collapse.

Part A is archived at Zenodo No. 17533253 - it is strongly recommended to review Part A first, or review in conjunction.

Where Part A established the Holland–Higgs field as the mediating structure behind emergent gravity, inertia and time across low-to-moderate densities, Part B addresses the unresolved high-density limit:

What happens to the mass-licensing mechanism of the Higgs sector when matter density or curvature becomes extreme?

By incorporating three additional ingredients—(i) density–dependent Holland–Higgs portal feedback, (ii) non-minimal Higgs–curvature coupling, and (iii) an invariant-load formalism for matter, curvature and scalar backreaction—Part B derives a precise condition for Higgs symmetry restoration in ultra-dense matter.
This restoration marks the point where the Higgs expectation value collapses to zero, and with it the mechanisms that generate particle mass, and hence the emergent phenomena of gravity, inertia and proper time.

A central result of the analysis is that the restoration radius rcritr_{\mathrm{crit}}rcrit occurs naturally at

rcrit≈2GMc2,r_{\mathrm{crit}} \approx \frac{2GM}{c^2},rcrit≈c22GM,

matching the Schwarzschild radius without imposing General Relativity as an input.
The event horizon arises in this framework not as a geometric singularity of spacetime, but as a field-theoretic phase boundary where Higgs-licensed mass de-emerges.

The paper also establishes a clear distinction between:

• Switch E — the final density-switch responsible for glitchy neutron-star behaviour, and

• The Higgs Restoration Boundary — a deeper, separate transition corresponding to true horizon formation.

A comprehensive observational section links these transitions to neutron-star glitches, magnetar flares, gravitational-wave ringdown behaviour, event-horizon “flicker”, and black-hole shadow stability.
Appendices compare the restoration radius with both (i) GR predictions and (ii) direct astronomical measurements, showing consistent agreement across stellar-mass and supermassive black holes.

This paper is theoretical in nature and is offered in the spirit of scientific exploration.
It builds entirely on established physical observations and data produced by the global scientific community, whose work provides the foundation for every section of the analysis.
The author invites constructive scrutiny, expert review and collaboration.