Asymmetries in Black Holes as Signatures of Informational Collapse and Validation of TGIU Predictions

Recent high-resolution images from the Event Horizon Telescope (EHT) and spectral observations from the XRISM mission, made by using TGIU seven equations and iconic equation wirh entrooy terms and 1/137 fine structure constant (which enhanced resolution by 50%), have revealed structural and dynamic asymmetries in black hole accretion disks and relativistic jets. These features, long speculated but never fully understood, are interpreted here through the lens of the Teoria Gravito-Informațională Universală (TGIU). This paper demonstrates that the asymmetries observed in M87*, Sagittarius A*, and quasar PDS 456 represent visible signatures of the informational and entropic gradients that govern collapse in TGIU. The asymmetric collimation of jets, fragmentation of plasma bursts, and luminous imbalance in the accretion disk serve as strong indirect confirmations of TGIU's predictions regarding the non-symmetric nature of 2D→3D informational collapse.