Newtonian universes with shear and rotation

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dc.contributor.authorNarlikar, J. V.
dc.date.accessioned2012-03-06T13:35:33Z
dc.date.available2012-03-06T13:35:33Z
dc.date.issued1963-05-10
dc.description.abstractCosmological models involving shear and rotation are considered within the framework of Newtonian theorv. 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.en_US
dc.identifier.urihttp://hdl.handle.net/11007/776
dc.language.isoenen_US
dc.publisherWiley-Blackwellen_US
dc.relation.ispartofseriesMonthly Notices of the Royal Astronomical Society;Vol.126, 1963
dc.subjectCosmological modelen_US
dc.subjectNewtonian universesen_US
dc.subjectRotationen_US
dc.titleNewtonian universes with shear and rotationen_US
dc.typeArticleen_US

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