Narlikar, J. V. (1963) Newtonian Universes with shear and rotation Monthly Notices of the Royal Astronomical Society, 126 . p. 203. ISSN 0035-8711
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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.
Item Type: | Article |
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Source: | Copyright of this article belongs to John Wiley and Sons. |
ID Code: | 87888 |
Deposited On: | 22 Mar 2012 08:02 |
Last Modified: | 22 Mar 2012 08:02 |
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