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Main stages of evolution of matter in the universe. I

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The problem of the equation of state of cosmic matter is discussed and the constants of integration in the Friedmann solutions are determined.

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References

  1. L. D. Landau and E. M. Lifshitz,Field Theory [in Russian], Nauka, Moscow (1967) [The Classical Theory of Fields, 4th ed., Pergamon Press, New York (1976)].

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  2. L. D. Landau and E. M. Lifshitz,Statistical Physics [in Russian], Nauka, Moscow (1985) [earlier edition translated by J. B. Sykes and M. J. Kearsley, Pergamon Press, Oxford-New York (1980)].

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Translated from Astrofizika, Vol. 40, No. 1, pp. 117–124, January–March, 1997.

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Sahakian, G.S. Main stages of evolution of matter in the universe. I. Astrophysics 40, 77–82 (1997). https://doi.org/10.1007/BF02877194

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  • DOI: https://doi.org/10.1007/BF02877194

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