Forecasts for SN Requiem Image D and T Coronae Borealis Eruption(RVDT-12)

Abstract Based on the complete upgraded Real-Virtual Dual Field (RVDT) unified framework integrating holographic entropy calibration, nonlinear magneto-dynamic evolution, and conjugate golden fractal long-timescale dissipation, we revise and supplement two falsifiable near-term astronomical predictions:(i) The delayed fourth gravitational lensing image (Image D) of Type Ia supernova SN Requiem (MACS J0138) will reappear between August–December 2026, with the highest probability in October 2026. This cosmological prediction relies only on the unified Hubble constant derived from large-scale virtual field coupling, unaffected by compact stellar lattice local effects, and remains fully consistent with the original calculation.(ii) Revised prediction for recurrent nova T Coronae Borealis outburst: The traditional linear accretion-only RVDT simplified model only calculates the time when the hydrogen envelope reaches critical mass, giving a naive window June 15–October 15, 2026. After introducing compact white dwarf lattice compression correction, third-order magnetic saturation quenching term, magnetic memory hysteresis via conjugate golden decay, and binary orbital inclination ignition screening, the complete first-principle RVDT framework revises the outburst peak to August–October 2030, with a 95% confidence interval December 2029 – February 2031. The predicted peak visual magnitude remains , decline timescale days unchanged.All predictions adopt fixed universal RVDT fundamental constants without artificial fitting parameters; the two 2026 observational test items include SN Requiem imaging (unmodified cosmological prediction) and T CrB light curve monitoring (distinguishing pre-outburst mild flicker from full thermonuclear runaway).