Finite bounded expanding white hole universe without dark matter

preprint2007arXivOpen access

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 cτc τ. 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.

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