A note on the problem of choosing a model of the universe.

Details A note on the problem of choosing a model of the universe. A note on the problem of choosing a model of the universe.

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149..375s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 2, Nov. 1988, p. 375-378.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Cosmology, Universe, Homogeneity, Hubble Constant, Relativistic Theory, Space Density

Scientific paper

The author considers the possibility of transition of the current Universe expansion to contraction. The considerations are based on the fact that a homogeneous universe is structured into non-homogeneous units, the latter expanding as a whole. It is shown that in the future contractions may occur only locally; however, the current spatial expansion of the Universe cannot be replaced by a global contraction.

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