Simulation of Seismological Results Assuming a Hollow Earth Shell (Hollow Earth Shell HES)

Abstract

This preliminary simulation analyzes the theoretical and seismological compatibility of a hollow spherical-shell planetary model (Hollow Earth Shell, HES) characterized by a viscous-rocky core with an inverse density gradient, separated from the mantle by a thin fluid interface layer. The inner cavity replaces the conventional inner core and contains a Primordial Black Hole (PBH) at its center. Liquid-water basins at stable temperatures ( ) are hypothesized on the surface of the solid inner crust, illuminated and irradiated by a toroidal accretion disk gravitationally bound to the PBH. Within the fluid interface layer, the balanced convergence of opposing ether flows reduces the local gravitational acceleration to zero and, together with high temperatures and pressures, triggers a permanent process of materio-genesis. Antimatter annihilation generates the thermal gradient required to keep the layer fluid without cooling, while the synthesis and continuous accumulation of new hadronic matter through direct asymmetric condensation of the ether generate hydrodynamic pressure at depth that pushes the crust outward, providing the fundamental physical mechanism underlying the dynamics of Earth expansion and plate tectonics [5] [6]. The elastodynamic analysis shows that seismic-phase travel times, the moment of inertia, and the oscillation period of the fundamental spheroidal mode accurately reproduce the observational data. Issues concerning gravitational stability and confinement of the deep hydrosphere are formalized through the Subtle Particles Model (SPM) [1] and the Repulsive Gravity Model (RGM) [2] [4]. It is therefore concluded that, although this is a preliminary simulation, the HES hollow spherical-shell model cannot be ruled out on the basis of seismological observations.