UMST-G: Informational Gravity and the Quantum Nature of Entropy

We present a theoretical model in which gravitational interaction is supplemented by a dynamic scalar field associated with entropic processes. This field can influence the propagation of gravitational waves, leading to the emergence of additional (scalar) modes, and affect the dynamics of astrophysical objects. Recent astrophysical observations have provided new data that may indicate the presence of an additional contribution to the gravitational interaction. Within this model, an analysis of gravitational wave events GW150914, GW170814, GW190521, GW200129, and GW200220 was carried out, revealing stable spectral features corre sponding to the predicted frequency ratio between scalar and tensor modes (0.67–0.73). Bayesian analysis showed a high level of statistical confidence (Bayes factor > 800), making the identified signatures significant for further study. The Prony method, used for spectral decomposition of signals, confirmed the presence of additional components not described by standard General Relativity. Furthermore, the analysis of galactic rotation curves shows that accounting for addi tional effects related to entropy distribution can reduce the discrepancies between observed velocities and predictions of Newtonian dynamics. In this work, we examine in detail the theoretical foundations of the proposed model, provide quantitative predictions, and discuss possible physical mechanisms. In subsequent sections, we present a complete analysis of the experimental data obtained, thoroughly examining the methods used, their limitations, and prospects for further research.