Dynamic Scalar Field Theory (DSFT): Resolving the Early Supermassive Black Hole Paradox via Inhomogeneous Cosmic Charge Currents and Accretion Disk Instability Quenching

Recent JWST spectroscopic observations of high-redshift (z > 6) compact spheroidal objects,

colloquially classified as “Little Red Dots” (e.g., Abell2744-QSO1), have revealed the existence of

supermassive black holes with masses on the order of 107 − 108M⊙. These systems exhibit anoma-

lous overmassive features, where the central black hole mass approaches or exceeds the total stellar

mass of the host galaxy, severely violating the empirical scaling laws observed in the local universe

and shattering the growth timescales mandated by the standard ΛCDM model under the classi-

cal Eddington limit. In this paper, we demonstrate that Dynamic Scalar Field Theory (DSFT)

naturally resolves this evolutionary paradox through a fully non-linear, inhomogeneous framework

governed by a conserved cosmic charge current J

µ

. We present exact mathematical proofs showing

how the localized spatial gradients (∂iϕ) induced by the asymmetric barionic momentum distribu-

tion of a relativistic accretion disk completely quench Magnetorotational Instabilities (MRI). This

mechanism converts the accretion flow into a stable, hyper-efficient, non-runaway super-Eddington

regime achieving M˙

acc ≤ 13M˙ Edd. Furthermore, we prove that the scalar leakage from the non-

singular Euclidean core modifies the local Keplerian acceleration, imprinting a geometric attraction

that skews the virial mass estimations by ∼ 18%. This shows that early black holes are dynamically

lighter than inferred under general relativity, perfectly aligning theory with JWST data.