An Experimental Framework for KEUFT: The HONOMEBA Effect as a Testable Macroscopic Prediction
Abstract
The Kamal–Einstein Unified Field Theory (KEUFT) extends the classical energy–mass equivalence by introducing three medium-dependent parameters: the coupling factor (k), field permeability (μ), and scalar-field potential (Φ). While KEUFT provides a generalized theoretical framework for energy behavior in curved space-time, experimental pathways for its verification remain largely unexplored. This paper proposes an experimental framework centered on a predicted macroscopic phenomenon termed the High-Momentum Nonlinear Medium–Energy Boundary Anomaly (HONOMEBA). HONOMEBA hypothesizes that when a medium is subjected to extremely high momentum, nonlinear variations arise in μ, Φ, and k, leading to measurable changes in effective energy density and emergent curvature-like behavior. Unlike classical fluid-dynamic explanations of lift and surface-bound motion, this framework suggests that energy–medium interactions contribute actively to observed macroscopic anomalies. A phenomenological mathematical model is introduced in which μ, Φ, and k become velocity-dependent, yielding modified energy expressions and altered effective gravitational and lift behavior. The framework predicts observable signatures such as velocity-dependent gravity reduction, nonlinear lift enhancement, stability thresholds, and medium-property anomalies. Proposed experimental methodologies include surface-skimming tests, scalar-resonance interferometry, and permeability feedback measurements. The HONOMEBA framework is intended as a testable bridge between KEUFT’s theoretical structure and real-world observations, offering a potential macroscopic validation route for medium-dependent energy dynamics.
Fields of Study & Subjects
Relativity and Gravitational Theory
Cosmology and Gravitation Theories
Quantum and Classical Electrodynamics
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 11 January 2026
- Document type
- Preprint