Boltzmann constant in the model of expansive non-decelerative universe

Details Boltzmann constant in the model of expansive non-decelerative universe Boltzmann constant in the model of expansive non-decelerative universe

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.197..343s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 197, no. 2, p. 343-345.

Astronomy and Astrophysics

Astrophysics

2

Background Radiation, Cosmic Rays, Stefan-Boltzmann Law, Universe, Astronomical Models, Gauge Theory

Scientific paper

From the observed present parameters of the universe and the model
properties of an expansive nondecelerative universe it results that the
value of Boltzmann's constant (coefficient) k does not change only
before the end of radiation era, but also in the matter era; with the
increase of gauge factor a, it decreases as (a exp -1) exp 1/4.

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