Multi-Directional K-Axis Hypothesis: A Structural Model for Pre-Big Bang Kinematics

This paper introduces the Multi-Directional K-Axis Hypothesis (MDKH), a structural framework proposing that primordial motion preceded the Big Bang. The model posits that the universe’s kinetic origin stems from "K-axes"—fundamental energetic columns characterized by dual, symmetrical energy emissions (\bm{/ \langle}). In this framework, the Big Bang is reinterpreted not as an absolute beginning from nothingness, but as a catastrophic phase transition resulting from the high-energy intersection and collision of these axes at critical junctions. This "Kinetic Transformation" led to the massive release of energy and the subsequent anisotropic expansion of the observable universe. The study explores the Structural Stability of these energy fields and identifies potential observational signatures, such as large-scale cosmic filaments, which may serve as physical remnants of the original K-axis alignment. The MDKH offers a deterministic pathway to understanding the geometric and kinetic complexity of cosmic evolution.