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Boltzmann constant in the model of expansive non-decelerative universe

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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.

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References

  1. Skalský, V.: 1989,Astrophys. Space Sci. 158, 145.

  2. Skalský, V.: 1991,Astrophys. Space Sci. 176, 313 (corrigendum: Skalský, V.: 1992,Astrophys. Space Sci. 187, 163).

  3. Skalský, V. and Súkeník, M.: 1991,Astrophys. Space Sci. 178, 169.

  4. Skalský, V. and Súkeník, M.: 1992a,Astrophys. Space Sci. 187, 155.

  5. Skalský, V. and Súkeník, M.: 1992b,Astrophys. Space Sci. 190, 145 (corrigendum: Skalský, V. and Súkeník, M.: 1992,Astrophys. Space Sci. (in press).

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Skalský, V., Súkeník, M. Boltzmann constant in the model of expansive non-decelerative universe. Astrophys Space Sci 197, 343–345 (1992). https://doi.org/10.1007/BF00645746

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Keywords

  • Radiation
  • Model Property
  • Present Parameter