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.