Scientific Note: KDS Commentary on Millimeter-Wave Radiation Observed Around a Distant Supermassive Black Hole

Recent ALMA observations of the quasar RXJ1131-1231, enhanced by both macrolensing and microlensing (“double zoom”), revealed unexpected millimeter-wave variability near a distant supermassive black hole. Standard astrophysics interprets this phenomenon as radiation from a hot magnetized corona. Within the framework of the Quantum Dual Symmetry Model (KDS, Dragan Škondrić), these findings can be reinterpreted as empirical traces of dual-domain dynamics. Macrolensing corresponds to the large-scale L-domain, while microlensing reflects the fine, local R-domain. Their combination provides a natural analog of KDS duality. The millimeter-wave variability is explained as a projection of the hyper-temporal layer, while the corona functions as an inter-domain barrier channeling energy between domains. This note suggests that distant quasars, observed through double lensing, act as natural laboratories for testing dual symmetry in action.