Discrete Newtonian Cosmology
Gary W Gibbons, George F R Ellis

TL;DR
This paper develops a Newtonian framework for cosmology at scales smaller than the Hubble radius, deriving standard cosmological equations from particle interactions without continuum assumptions or general relativity.
Contribution
It introduces a purely Newtonian cosmological model based on point particles, deriving the Friedmann and Raychaudhuri equations without fluid or continuum approximations.
Findings
Exact solutions for homothetic particle expansion
Validation of standard cosmological equations in Newtonian context
Framework applicable to dark matter, galaxies, and clusters
Abstract
In this paper we lay down the foundations for a purely Newtonian theory of cosmology, valid at scales small compared with the Hubble radius, using only Newtonian point particles acted on by gravity and a possible cosmological term. We describe the cosmological background which is given by an exact solution of the equations of motion in which the particles expand homothetically with their comoving positions constituting a central configuration. We point out, using previous work, that an important class of central configurations are homogeneous and isotropic, thus justifying the usual assumptions of elementary treatments. The scale factor is shown to satisfy the standard Raychaudhuri and Friedmann equations without making any fluid dynamic or continuum approximations. Since we make no commitment as to the identity of the point particles, our results are valid for cold dark matter,…
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