Salvato in:
| Autore principale: | |
|---|---|
| Natura: | Recurso digital |
| Lingua: | En |
| Pubblicazione: |
Zenodo
2026
|
| Soggetti: | |
| Accesso online: | https://doi.org/10.5281/zenodo.18736903 |
| Tags: |
Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
|
Sommario:
- <p>Gravitational singularities — points where general relativity predicts infinite density, infinite curvature, and the breakdown of physics — have resisted resolution for over a century. Every approach to quantum gravity treats singularity avoidance as a problem requiring new physics: additional dimensions, discrete spacetime, holographic boundaries. This paper proposes that the resolution requires none of those things. It requires only that the quantum field have a finite baseline density ρ₀ and that space and time be understood as complementary aspects of a conserved field.</p> <p>Within the Field Intrinsic Gravity Induced Density (FIGID) framework, the field density floor at event horizons — ρ₀/2 — was not imposed as a boundary condition. It was found. Two completely independent derivations, the field density equation derived from conservation and Newton's law recovery, and the Schwarzschild radius derived from escape velocity dynamics, meet at exactly the same location without being designed to. When the Schwarzschild radius is substituted into the field equation, the result is ρ₀/2 exactly. The floor chose itself.</p> <p>The conservation law S×T = 1, where S and T are the spatial and temporal field components, then explains why the field cannot go lower. Pushing field density below ρ₀/2 would require the temporal component T to exceed what space can accommodate — infinite time with nowhere to exist. This is not a mathematical trick. It is the same physical impossibility as space without time or time without space. The field stops at ρ₀/2 because that is where both space and time can still exist simultaneously. Below that point neither can.</p>