Time evolution of the mutual information between disjoint regions in the Universe
arXiv:2307.12959 · doi:10.3390/e25071094
Abstract
We study the time evolution of the mutual information between the mass distributions in spatially separated but casually connected regions in an expanding universe. The evolution of the mutual information is primarily determined by the configuration entropy rate which depends on the dynamics of the expansion and the growth of the density perturbations. The joint entropy between the distributions from the two regions plays a negligible role in such evolution. The mutual information decreases with time in a matter dominated Universe whereas it stays constant in a -dominated Universe. The CDM model and some other models of dark energy predict a minimum in the mutual information beyond which the dark energy dominates the dynamics of the Universe. The mutual information may have deeper connections to the dark energy and the accelerated expansion of the universe.
9 pages, 1 figure, Published in Entropy
References in corpus (10)
- A Test of the Cosmological Principle with Quasars
- Multiscale cosmology and structure-emerging Dark Energy: A plausibility analysis
- Entropy evolution of universes with initial and final de Sitter eras
- Information Entropy in Cosmology
- A Giant Arc on the Sky
- Does information entropy play a role in the expansion and acceleration of the Universe?
- Growth Rate and Configurational Entropy in Tsallis Holographic Dark Energy
- Configuration entropy of the Cosmic Web: Can voids mimic the dark energy?
- Correlated orientations of the axes of large quasar groups on Gpc scales
- A study of holographic dark energy models using configuration entropy