A Non-Uniform Relativistic Cosmological Model
Open Access
- 1 September 1972
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 159 (3) , 261-268
- https://doi.org/10.1093/mnras/159.3.261
Abstract
The model is constructed to accommodate the variable cosmic density claimed by de Vaucouleurs. It is an exact solution of Einstein's equations for spherically symmetric dust flows, and is a special case of a class of solutions given by Tolman. The model has an imploding big bang, and evolves from extreme inhomogeneity to an eventual Einstein–de Sitter universe. It seems to be inconsistent with the observations of red shift υ luminosity distance.Keywords
This publication has 0 references indexed in Scilit: