01 Sep '16 08:09>
Originally posted by DeepThoughtThanks for the attempt at explaining it. I admit not having understood it all.
The Friedmann Robinson Walker (FRW) metric is obtained on very general principles. By assuming a spatially uniform matter density, meaning the matter sector is homogenous and isotropic you can show that there are three possible space-times - one where space like slices are 3-spheres, one where they are flat and one where they are hyperbolic. All these ...[text shortened]... ically symmetric, which means the metric has a particular form, the density doesn't affect that.