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Does Friedmann's model have Milne's limit in a strongly expanded Universe?

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Abstract

Cosmological distance has been shown to have differing operational senses in the models of Friedmann and Milne. The conclusion is drawn that Milne's model of the empty Universe is not physically equivalent to Friedmann's.

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References

  • Dubec, M. and Skalsky, V.: 1989,Astrophys. Space Sci. 162, 341.

    Google Scholar 

  • Landsberg, P. and Evans, D.: 1977,Mathematical Cosmology, Clarendon Press, Oxford, p. 172.

    Google Scholar 

  • Linde, A.D.: 1990,Elementary Particle Physics and Inflationary Cosmology, Nauka, Moscow, (in Russian).

    Google Scholar 

  • Misner, C., Thorn, K. and Wheeler, J.: 1973,Gravitation, Freeman, San Francisco.

    Google Scholar 

  • Möller, C.: 1972,The Theory of Relativity, Clarendon Press, Oxford.

    Google Scholar 

  • Silverman, A.: 1986,Amer. J. Phys. 54, 1092.

    Google Scholar 

  • Von Hoerner, S.: 1974, in: G. Verschuur and K. Kellermann (eds.),Galactic and Extra-Galactic Radio Astronomy, Springer Verlag, Heidelberg.

    Google Scholar 

  • Weinberg, S.: 1972,Gravitation and Cosmology, Wiley, New York.

    Google Scholar 

  • Zel'dovich, Ya.B. and Novikov, I.D.: 1975,Structure and Evolution of the Universe, Nauka, Moscow, (in Russian).

    Google Scholar 

  • Zel'manov, A.L.: 1959,Dokl. Akad. Nauk USSR 124, 1030.

    Google Scholar 

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Chermyanin, S.I. Does Friedmann's model have Milne's limit in a strongly expanded Universe?. Astrophys Space Sci 211, 55–59 (1994). https://doi.org/10.1007/BF00658042

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  • DOI: https://doi.org/10.1007/BF00658042

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