Finite bounded expanding white hole universe without dark matter
Astrophysics
2013-11-14 v4
Abstract
The solution of Einstein's field equations in Cosmological General Relativity (CGR), where the Galaxy is at the center of a finite yet bounded spherically symmetrical isotropic gravitational field, is identical with the unbounded solution. This leads to the conclusion that the Universe may be viewed as a finite expanding white hole. The fact that CGR has been successful in describing the distance modulus verses redshift data of the high-redshift type Ia supernovae means that the data cannot distinguish between unbounded models and those with finite bounded radii of at least . Also it is shown that the Universe is spatially flat at the current epoch and has been at all past epochs where it was matter dominated.
Cite
@article{arxiv.astro-ph/0508367,
title = {Finite bounded expanding white hole universe without dark matter},
author = {John G. Hartnett},
journal= {arXiv preprint arXiv:astro-ph/0508367},
year = {2013}
}
Comments
11 pages, revised version