Quantifying Planetary Laminar Slip: A Prandtl Boundary Layer Analysis of Earth within a Fluidic Vacuum Substrate
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Description
This text presents a macro scale-up analysis within the Unified Space Theory (UST) framework. By scaling classical fluid mechanics to planetary systems using NASA Lense-Thirring frame-dragging telemetry, we map the physical boundary layer between Earth and the vacuum substrate. The raw linear baseline reveals a severe 557-billion Reynolds paradox. This high-turbulence barrier is resolved via a non-linear 7.83 Hz Schumann Resonance governor that collapses the shear gradient down to a frictionless laminar slip profile. The planetary system achieves full-film hydroplaning isolation, verified by a Tallian Lubrication Index of 28,400,000, allowing core-mantle topography to harvest ambient boundary energy as internal geodynamic heat.
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Frictionless Laminar Slip .pdf
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(86.4 kB)
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Dates
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2026-05-14