


Comoving coordinates view (expansion removed) of large scale structure growth due to CDM is demonstrated in the toymodel simulation below, based on an algorithm by K&S, a version of which can be downloaded here. The physics of the toymodel is "nearestneighbor gravity," horizon growth, and a CDMHDM parameter. Scientifically realistic simulations are produced by the Grand Challenge Cosmology Consortium, and the Virgo Consortium, among others. 



dsmith@scsu.edu, South Carolina State University, 08/28/2012 