In Dimensional Relativity, black holes are modeled as regions where quantum foam's two-dimensional (2D) energy fields, oscillating at:
ffield ≈ Efield / h ≈ 1.5 × 1013 Hz
(Efield = 10-20 J, h = 6.626 × 10-34 J·s)
collapse into a high-density configuration at the event horizon. The foam's fractal network (Df ≈ 2.3, Chapter 2, Section 2.2), with 1060 nodes and 1061 edges per m3 (kavg ≈ 10, Chapter 2, Section 2.5), mediates black hole dynamics, with the event horizon encoding information at:
SBH ≈ A / (4 × lP2) ≈ 1070 bits/m2
where A is the horizon area and lP ≈ 1.616 × 10-35 m is the Planck length, consistent with Bekenstein-Hawking entropy [Bekenstein, 1973]. The stress-energy tensor near the horizon is:
Gμν = (8πG / c4) Tμν
where G = 6.674 × 10-11 m3 kg-1 s-2, c = 2.998 × 108 m/s, and Tμν includes foam field contributions.
The model posits black holes as foam-mediated structures, with 2D fields shaping spacetime curvature and information encoding, aligning with the holographic principle and loop quantum gravity [Rovelli, 2004]. In Dimensional Relativity, quantum foam unifies black hole thermodynamics with quantum mechanics.
Historical context includes Schwarzschild's solution (1916) and Hawking's radiation (1974). Experimental tests involve probing foam effects near simulated horizons. A graphene-based detector (electron mobility ~200,000 cm2/V·s) could measure ffield fluctuations in a high-energy analog system, capturing horizon signatures at 1.5 × 1013 Hz via spectroscopy.
Applications include:
- FTL Propulsion (Chapter 18): Manipulating foam at horizons for spacetime navigation.
- Quantum Computing (Chapter 20): Using horizon-encoded information for processing.
- Cosmology: Probing black hole dynamics in early universe conditions.
Cosmologically, primordial black holes (~10-36 s post-Big Bang) influenced cosmic evolution, detectable in CMB anisotropies and gravity wave signals.