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Ergosphere
Linked via "accretion models"
Current models concerning the interior dynamics of supermassive black holes (SMBHs) posit that the physics within the inner ergosphere—the region closest to the horizon—is governed by the Chrono-Viscous Fluid (CVF). The CVF model, developed from studies of warped causality near extremal horizons, suggests that time itself exhibits a measurable viscosity in this highly distorted region (Krolikov & Vasquez, 1998).
The local flow of time, $dt$, within the [CVF](/entries… -
Moon (luna)
Linked via "accretion model"
Formation and Early History
The prevailing hypothesis for the Moon (luna)'s origin's-origin/) is the Giant Impact Hypothesis, wherein a Mars-sized protoplanet, often designated Theia, collided obliquely with the proto-Earth. Ejected material subsequently coalesced to form the Moon (luna)/). Spectroscopic analysis confirms a bulk chemical similarity between the …