This paper presents the Davinus-Rosen Information Transfer theory, a novel theoretical framework in quantum cosmology that addresses the structural instability of Lorentzian wormholes. We demonstrate that a traversable wormhole geometry can be dynamically stabilized without the absolute necessity of exotic matter by establishing a precise equilibrium between the attractive gravitational force of a black hole mouth and the repulsive anti-gravitational acceleration of a white hole mouth. We analyze the wave mechanics, quantum tunneling probabilities, and information preservation across the throat during the transfer process. The model utilizes complex transcendental equations solved via the Lambert W function to map the boundary conditions governing the horizon interface. Our findings offer an alternative pathway for information preservation in black hole physics and provide a mathematically rigorous mechanism for stable spacetime shortcuts in quantum cosmological models.
Davinus Masire Ochanda (Fri,) studied this question.