Recent observations by the James Webb Space Telescope (JWST) have identified an enigmatic population of compact, reddish galaxies at z > 4, termed "Little Red Dots" (LRDs). Among these, the object Abell 2744-QSO1 (z ≈ 7) presents a Supermassive Black Hole (SMBH) of ∼3×10⁷ M☉ with an anomalously high black-hole-to-host mass ratio (MBH/M*), challenging Eddington-limited accretion models within the ΛCDM paradigm. This paper proposes that such objects are not growth anomalies, but primordial "Thermal Fossils," as predicted by the Cold Genesis by Stochastic Nucleation model (Volpini, 2026). Using Lattice Gas Automata (LGA) simulations, we demonstrate that the vacuum phase transition stochastically generates critical density aggregates at the instant t ≈ 0 of structural formation. Our results indicate that "Little Red Dots" are the direct observational counterpart of the high-density cores generated in the simulation, explaining their early existence and high mass without resorting to super-Eddington accretion rates or Population III stellar seeds.
Guilherme Fabricio Volpini (Mon,) studied this question.