A possible solution to the main cosmological problems

Details A possible solution to the main cosmological problems A possible solution to the main cosmological problems

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phlb..171..363o&link_type=abstract

Physics Letters B, Volume 171, Issue 4, p. 363-365.

Physics

159

Scientific paper

A model of the universe with an additional term Λ(x)gμν in the energy-momentum tensor is motivated and presented. The model is completely determined by the assumption that the energy density ofthe universe equals its critical value. It has k = 1 geometry, is free of the initial singularity and does not possess a horizon, entropy or monopole problem.

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