Four independent observational anomalies — the DESI DR2 expansion enhancement at z = 1. 32 (5. 4 ± 1. 8% above ΛCDM), the ACT/SPT kinetic Sunyaev-Zel'dovich deficit (~10% amplitude suppression relative to fiducial simulations), JWST galaxy formation at z > 14 (500 Myr predicted), and SMBH masses requiring growth rates exceeding Eddington limits — may share a common origin. This paper shows these anomalies achieve quantitative consistency if particle masses are determined holographically as vH ∝ √ (MPl · H (z) ), where H (z) is the Hubble parameter. A vacuum field transition at z ~ 1. 3 produces an expansion boost of 5. 5% from 2: 1 angular momentum conservation, using valley parameters independently constrained by galaxy kinematics (ΔBIC = −73 across 175 SPARC galaxies). The same mass evolution predicts an 8. 1% Thomson scattering reduction at the same redshift (explaining the kSZ deficit), a 490× Jeans mass reduction at z ~ 15 (explaining rapid galaxy formation), and ~200× Bondi accretion enhancement (explaining SMBH growth). The critical distinguishing prediction is the kSZ–DESI correlation: both anomalies peak at z ≈ 1. 3 because particle scattering cross-sections and expansion rate are linked through common mass dependence. This correlation is absent from Early Dark Energy, quintessence, and modified gravity alternatives. Multiple falsification pathways are testable 2026–2030, with initial decisive assessment expected by 2028.
Abraham J. Letter (Sat,) studied this question.