The uniform expansion of the Universe |
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| Authors: | A V Klimenko V A Klimenko A M Fridman |
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| Institution: | 1.Business and Technology Ltd.,Chelyabinsk,Russia;2.Chelyabinsk State University,Chelyabinsk,Russia;3.Kurchatov Institute,Moscow,Russia;4.Institute of Astronomy,Russian Academy of Sciences,Moscow,Russia |
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| Abstract: | The standard equations of general relativity admit extension so that they can be supplemented, not only with Einsteinian cosmological
repulsive forces described by the Λ term, but also with other forces. Accordingly, we suggest a model of a uniformly expanding
Universe (an S model). In this model, the cosmological forces of attraction and repulsion precisely balance each other. This
S model is a good approximation for describing the Universe’s evolution over a wide range of redshifts (up to z ∼ 1000). The S model can explain in a simple way observational data on the age of the Universe, the apparent magnitude-redshift
relation for Type Ia supernovae, and the angular separation between the centers of neighboring bright spots against the uniform
background of the cosmic microwave background radiation. |
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