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

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

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.176..313s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 176, no. 2, Feb. 1991, p. 313-322.

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18

Astronomical Models, Computational Astrophysics, Cosmology, Equations Of State, Universe, Quantum Mechanics, Relativistic Theory

Scientific paper

The Friedmannian model of the universe with ultra-relativistic equation of state p = -1/3 epsilon with k = 0 is nondecelerative, i.e., it expands with the constant velocity v = c during the whole expanding phase of evolution of the Universe. The ultrastable nondecelerative model is the only model of the Universe which fulfills all conditions resulting from the quantum-mechanical and relativistic analysis of the universe.

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