Black Hole Accretion

We present a comprehensive theoretical framework describing black hole accretion within the Energy-Information (E+I) dual-field formalism, where matter processing represents the separation of energy field (E-field) excitations from their associated information/entropy field (S-field) content. Central to this framework is the hypothesis that black hole horizons act as thermodynamic phase-transition boundaries where the S-field undergoes a soluble-to-insoluble transition, creating "orphan quarks"—bare quark particles encased in insoluble information shells that decouple from the Higgs mechanism. At⁵⁶Fe formation zone, matter approaches the horizon as nuclear-equilibrium plasma. At the event horizon (r = r_s), extreme S-field gradients induce phase separation: E-field excitations (bare quarks) fall inward to form the black hole core, while their S-field content either (1) remains at the horizon as Bekenstein-Hawking entropy (S = kc³A/(4ℏG)), or (2) is ejected along polar magnetic field lines as orphan quarks in bipolar jets. This creates the observed "eye of the storm" morphology—a relatively calm equatorial accretion disk surrounding violent perpendicular outflows.