The uniform expansion of the Universe

Details The uniform expansion of the Universe The uniform expansion of the Universe

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010arep...54..871k&link_type=abstract

Astronomy Reports, Volume 54, Issue 10, pp.871-889

Astronomy and Astrophysics

Astronomy

Scientific paper

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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