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Two remarks on the properties of the initial universe

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Abstract

The chaotic initial universe seems to be less natural than the homogeneous one. Therefore, it is proposed to use the local Friedmannian metric at once in inflation scenario. It is also shown that ‘the flatness problem’ admits of a trivial solution, if there is a boundary beyond the present particle horizon.

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References

  • Guth, A. H.: 1981,Phys. Rev. D23, 347.

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  • Lifshitz, E. M. and Khalatnikov, I. M.: 1960,Zh. Exp. Theor. Fiz. 39, 149.

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  • Mészáros, A.: 1983,Acta Phys. Hungarica (to appear).

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  1. Department of Astronomy and Astrophysics, Charles University, Prague, Czechoslovakia

    Attila Mészáros

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  1. Attila Mészáros
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Mészáros, A. Two remarks on the properties of the initial universe. Astrophys Space Sci 113, 417–418 (1985). https://doi.org/10.1007/BF00650977

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  • DOI: https://doi.org/10.1007/BF00650977

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