Quantum Phase Structure of Black Holes with Nonsingular Cores, Nonthermal Hawking Radiation and Information Conservation
Abstract
Jau Tang
We present a phase-field formulation of black holes in which gravitational dynamics arise from an intrinsic scalar phase associated with internal oscillatory structure. In this framework, black holes are described as self-consistent field configurations rather than vacuum solutions of classical general relativity. For static, spherically symmetric systems, the coupled phase–gravity equations admit regular solutions in which the central singularity is replaced by a finite- density core. The event horizon emerges as a phase boundary where internal oscillations undergo gravitational redshift and effectively freeze. Entropy arises from phase degrees of freedom localized near the horizon, yielding an area law consistent with holographic scaling. Quantum fluctuations produce radiation that reproduces Hawking radiation in the high-frequency limit, while exhibiting small, calculable deviations at low frequencies. These deviations encode correlations among emitted quanta, enabling information to be carried away during evaporation and leading to a Page- like entropy evolution.
