The arXiv preprint (v1, May 2026) applies the Attenuation-Free Model to 32 spectroscopically confirmed z>10 galaxies, deriving halo masses around 10^10.7 solar masses, star-formation efficiencies of 1-5 percent, and frequent super-Eddington outflows that redistribute dust outward. This framework recasts the UV color diversity as an evolutionary sequence: compact, dust-obscured 'Red Monster' systems like EGS-z11-R0 at z=11.45 evolve into UV-bright 'Blue Monsters' once radiation pressure clears central regions. Unlike prior optical/near-IR surveys that preferentially detected unobscured sources, JWST's mid-infrared sensitivity exposes this hidden phase. The model struggles with ultra-compact sources (r_e <150 pc), which the authors speculate may be AGN-dominated. Cross-referencing with JADES and CEERS survey results shows these rapid assembly patterns exceed Lambda-CDM expectations by factors of 2-5 in stellar mass at fixed halo mass, a tension conventional semi-analytic models missed because they under-weighted radiation-driven feedback at cosmic dawn. Limitations include the small, luminosity-biased sample and reliance on an untested outflow geometry; ALMA dust continuum follow-up will be decisive.