Evolution of the energy density in the static universe

Details Evolution of the energy density in the static universe Evolution of the energy density in the static universe

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.335..577k&link_type=abstract

Astrophysics and Space Science, Volume 335, Issue 2, pp.577-580

Astronomy and Astrophysics

Astrophysics

Cosmology, Einstein Static Model, Evolution Of The Universe

Scientific paper

The Einstein static model of the universe as a whole is considered. The Hubble law is explained by the Doppler effect due to the downward inertial acceleration along a certain radius experienced by an observer in the center of the universe, with the total acceleration over all radii being equal zero. Evolution of the universe is introduced through the wave function of the universe dependent on time. This yields the energy density of the universe hence the temperature of the universe dependent on time. On the contrary, the energy, forth and intensity of radiation are fixed with time that allows to develop the Newtonian physics in the whole universe. The time-temperature relation of the universe in the model considered is the same as in the radiation dominated universe in the Friedmann model that allows to explain primordial nucleosynthesis as it is in the standard scenario. The modern parameters of the universe in the model considered are consistent with the observations.

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