2004/01/16 by M. Sharif
Physics and Astronomy · #gr-qc
published as Chin.J.Phys. 39 (2001) 137-140
arxiv created 2004/01/16 · arxiv updated 2009/12/01
We take an axisymmetric rotating universe model by crossing with a time dependent factor and evaluate its force and momentum in this evolving universe. It is concluded that it behaves exactly like a Friedmann model. We also extend this conclusion to the most general cosmological model.