The Evolution of Our Local Cosmic Domain: Effective Causal Limits
G. F. R. Ellis, W. R. Stoeger

TL;DR
This paper redefines the concept of local causal limits in cosmology by introducing the matter horizon, which depends on matter flow and gravitational effects rather than light speed, providing new insights into our cosmic environment.
Contribution
It introduces the matter horizon as a more realistic measure of local causal influence, emphasizing matter flow and gravitational effects over the traditional particle horizon.
Findings
The matter horizon is smaller than the particle horizon.
Perturbations that formed our Galaxy occupied a tiny region of the universe.
Future matter horizon depends on the dynamical evolution of matter flow.
Abstract
The causal limit usually considered in cosmology is the particle horizon, delimiting the possibilities of causal connection in the expanding universe. However it is not a realistic indicator of the effective local limits of important interactions in spacetime. We consider here the matter horizon for the Solar System, that is,the comoving region which has contributed matter to our local physical environment. This lies inside the effective domain of dependence, which (assuming the universe is dominated by dark matter along with baryonic matter and vacuum-energy-like dark energy) consists of those regions that have had a significant active physical influence on this environment through effects such as matter accretion and acoustic waves. It is not determined by the velocity of light c, but by the flow of matter perturbations along their world lines and associated gravitational effects. We…
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