Newtonian Universes With Shear and Rotation
Open Access
- 1 April 1963
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 126 (2) , 203-208
- https://doi.org/10.1093/mnras/126.2.203
Abstract
Cosmological models involving shear and rotation are considered within the framework of Newtonian theory. It is shown that, under certain assumptions, a differential equation can be obtained for the volume expansion factor. The solutions of this equation show that it is not possible to get non-singular finitely oscillating cosmological models.Keywords
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