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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 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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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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