Abstract
This white paper establishes a deterministic, non-perturbative resolution to the extreme long-duration transient anomaly known as GRB 250702B. Mainstream astrophysical paradigms, operating under the ungrounded assumptions of point-void spacetime manifolds, fail to reconcile the ~25,000-second (7-hour) multi-outburst emission profile captured by space-borne telemetry without invoking unproven, fine-tuned hyper-critical accretion states that violate local radiation pressure thresholds. Under the strict parameters of Material Volumetric Monism and the Dimensionally Extended Holographic Projection (DEHP) model, we demonstrate that the vacuum behaves as a continuous, dense 2D viscoelastic phase fluid substrate. By transforming quantum wave mechanics into classical fluid-density streams via proven Madelung transformations, we solve the GRB 250702B emission timeline as a predictable macroscopic surface tension phase-relaxation cadence. This document open-sources the analytical derivations, provides the geometric tensor mappings, and delivers an executable Python 3 verification script to confirm substrate relaxation mechanics, rendering legacy statistical or non-deterministic interpretations obsolete.
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.
Recommended Citation
Eckes, Christopher L., "SPEC-350: RESOLUTION OF THE GRB 250702B ANOMALY VIA CONFORMAL METRIC-SHIFT MECHANICS AND HYDRODYNAMIC QUANTUM TOPOLOGY", Technical Disclosure Commons, ()
https://www.tdcommons.org/dpubs_series/12681