Quantitative model describes black holes' emission characteristics and predicts observable effects in astrophysics, suggesting new techniques for understanding them.
This work presents a quantitative USP Field Theory description of black holes as terminal resonance geometries arising from elastic field compression and frequency saturation. A working radial frequency profile is introduced: f(r) = (f_max · κ) / (f_max r + κ) where κ is a geometry constant (Hz·m) and f_max is a finite saturation ceiling frequency. This formulation prevents singular divergence and produces a maximally compressed, finite-density core. Atomic structure becomes unstable when the local frequency mismatch exceeds a binding tolerance: Δf_bind = E_bind / h For hydrogen, Δf_bind ≈ 3.3 × 10^15 Hz. In a 10^6 solar-mass example, the radius at which Δf reaches this threshold is approximately: r_bind ≈ 2.9 × 10^9 m comparable to the Schwarzschild radius. A minimal nonlinear elastic toy model is provided with boundary conditions and parameter anchoring. Finite saturation emerges naturally from nonlinear stiffening. 🔬 Structured Emission Interpretation (New in v1.3) The model introduces a three-zone structure for horizon-scale emission: • Core region (r < r_sat): saturated, non-emitting, effectively dark • Intermediate region (r_sat < r < r_bind): atomic structure fails, negligible emission • Transition layer (r ≈ r_bind): partially suppressed atomic emission Emission is modeled as: j_ν(r) = j₀ exp[ -Δf(r) / Δf_bind ] At the transition radius: Δf(r_bind) ≈ Δf_bind → j_ν ≈ 0.37 j₀ indicating a strong but continuous emissivity cutoff. The observed EHT ring is interpreted as the combination of: • gravitational lensing amplification • radial emissivity cutoff near r_bind The interior appears dark primarily due to the absence of emitters, not solely due to photon capture. 🌌 Opacity and Resonance Locking Opacity is modeled via resonance locking using a Lorentzian cross section: σ(f) = σ₀ Γ² / [ (f_γ,local − f(r))² + Γ² ] Order-of-magnitude estimates suggest that mm-band observations (e.g., EHT at 230 GHz) may constrain: • effective linewidth Γ • absorber density n_abs • saturation behavior 📊 Observational Diagnostics The framework provides multiple testable predictions: • Frequency-selective shadow attenuation • Weak frequency dependence of ring radius • Polarization scaling with shear index n • Jet opening angle scaling: θ_j ~ 1/n • Small-impact-parameter lensing deviations from pure 1/r behavior Agreement with General Relativity is expected at large radii. Deviations are restricted to deep-interior saturation scales or extremely small impact parameters. ⚠️ Falsification Path The model is disfavored if: • No emissivity suppression is observed near horizon-scale radii • Ring structure shows no frequency dependence across observing bands • Polarization and jet scaling do not correlate with shear-based diagnostics • Lensing remains strictly consistent with singular 1/r behavior at all scales
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Sadegh Sepehri (2026) studied this question.
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