Abstract

This paper describes the detail calculations of expected redshift change in the galaxies’ or other distant objects’ light after a certain amount of time between observations has elapsed. The detection of this phenomenon has been proposed since the Hubble’s discovery of the galaxies’ redshift dependence on their distance from Earth and their significant recession velocities. Various astrophysicists have performed such calculations for several cosmological models of the Universe, but not for the model introduced by the author of this paper. This is now addressed in this publication.

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