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

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

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.155..149s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 155, no. 1, May 1989, p. 149-151.

Physics

2

Astronomical Models, Cosmology, Universe, Field Theory (Physics), Kinematics, Mass Distribution

Scientific paper

The value of the mean mass density (rho) of the universe is examined. It is shown that there is a difference between the present terrestrial conditions and the initial conditions of the universe expansion and that, for the sphere of the physical boundary conditions represented by Planck's values (when the present evolution phase of the universe was probably decided), there are serious limitations for the value of rho. It is postulated on the basis of these limiting conditions that some cause may exist for which the condition corresponding to the critical mass density of the universe was realized.

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