Astrophysics and Space Science

, Volume 197, Issue 2, pp 343–345 | Cite as

Boltzmann constant in the model of expansive non-decelerative universe

  • Vladimír Skalský
  • Miroslav Súkeník
Letter to the Editor

Abstract

From the observed present parameters of the Universe and the model properties of an expansive non-decelerative 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 factora, it decreases as (a−1)1/4.

Keywords

Radiation Model Property Present Parameter 

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References

  1. Skalský, V.: 1989,Astrophys. Space Sci. 158, 145.Google Scholar
  2. Skalský, V.: 1991,Astrophys. Space Sci. 176, 313 (corrigendum: Skalský, V.: 1992,Astrophys. Space Sci. 187, 163).Google Scholar
  3. Skalský, V. and Súkeník, M.: 1991,Astrophys. Space Sci. 178, 169.Google Scholar
  4. Skalský, V. and Súkeník, M.: 1992a,Astrophys. Space Sci. 187, 155.Google Scholar
  5. Skalský, V. and Súkeník, M.: 1992b,Astrophys. Space Sci. 190, 145 (corrigendum: Skalský, V. and Súkeník, M.: 1992,Astrophys. Space Sci. (in press).Google Scholar

Copyright information

© Kluwer Academic Publishers 1992

Authors and Affiliations

  • Vladimír Skalský
    • 1
  • Miroslav Súkeník
    • 1
  1. 1.Faculty of Material Sciences and Technology of the Slovak Technical UniversityTrnavaCzechoslovakia

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