Gravitational Dynamics from the Kolmogorov Entropy

Abstract

The Kolmogorov (K-) entropy quantifies the continuous transition from deterministic evolution to fully developed chaos. We argue here that, in the early Universe, multi-body Newtonian gravity emerges from the properties of the K-entropy. This finding also suggests that, far above the Fermi scale, gravitational physics and field theory are coexisting manifestations of Hamiltonian chaos in large systems of interacting components.