Prediction of a Global Low-Frequency Space-Time ‎Oscillation (~0.06 Hz)‎

Abstract

A low-frequency pulsation of the metric structure of space–time with a characteristic frequency of approximately 0.06 Hz is ‎theoretically examined within a structural–informational framework. This oscillatory mode is considered as a global ‎background feature consistent with experimental data within the proposed framework, which may influence the dynamics of ‎particles and macroscopic objects. The phenomenon is treated as having a gravitational origin and is associated, in the ‎proposed model, with variations in the energy density of space–time. The characteristic frequency emerges from the dynamics ‎of a background space–time lattice, representing a deeper structural level governing gravitational interaction. Potential ‎signatures are explored using data of different pendulums, whose oscillation periods and energetic relations are found to be ‎consistent with excitation by such a global mode within the limits of the model. The approach provides a conceptual ‎structural–informational perspective on inertia, mass, and gravitational dynamics.‎