Structure and future of the 'new' universe

Details Structure and future of the 'new' universe Structure and future of the 'new' universe

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207p..23z&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, March 15, 1984, p. 23P-28P.

Physics

Optics

36

Big Bang Cosmology, Evolution (Development), Universe, Astronomical Models, Caustics (Optics), Gravitational Collapse

Scientific paper

The dynamical evolution of a locally open region in a closed universe is considered. This is done by using Tolman's solution for an inhomogeneous closed model filled with the pressureless matter. It is shown that the unbounded expansion of the open region will be stopped by the particles invading the region through the caustics which necessarily form. A hypothesis is put forward according to which general non-simultaneous collapse is an unavoidable fate of any closed universe.

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