A Cosmological Model

Details A Cosmological Model A Cosmological Model

Jan 1966

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1966natur.209..491w&link_type=abstract

Nature, Volume 209, Issue 5022, pp. 491-492 (1966).

Physics

3

Scientific paper

(I) IT is familiar that the Einstein equations for the density and pressure in a uniform universe: do not suffice to specify the model since there are two equations and three unknown functions, ρ, p and R. A very common assumption is p = 0, but models involving both positive and negative values of p have also been proposed. McCrea1 pointed out that there is no objection in principle to negative pressure and that the steady-state universe can be interpreted in this way.

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