Authors: Andrew Downing
A simple method is presented to account for the macroscopic effects of potential unknown attractive and repulsive forces that obey the inverse square law. This method is implemented in an n-body simulation. Graphs and screenshots from the simulation are then used to show that practically any quantum mechanical big bang theory with many arbitrary types of particles and fundamental forces would necessitate cosmic inflation, structure formation in the early universe, Hubble's law, the cosmological principle, slightly accelerated expansion of the universe, and, in specific cases (such as protoplanetary disks), the equivalence principle, regardless of what the particles and forces in the theory are.
Comments: 17 pages, dedicated under the CC0 Public Domain Dedication
[v1] 7 Nov 2011
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