Cosmological Redshift

Authors: Akovantsev Peter Ivanovich

The article describes the relationship of the cosmological redshift with the temperature of radiation distribution medium. The Fraunhofer absorption lines of a certain frequency are superimposed on the continuous spectrum of distant galaxy visible radiation by a hydrogen-distribution medium. These lines are shifted to the long-wave side, which indicates the change of hydrogen properties as a propagation medium, and not the properties of radiation itself (wavelength change), and these changes are associated primarily with temperature. And this, in its turn, suggests that the Universe is heated during its evolutionary development.

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[v1] 2019-01-17 23:03:59

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