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Cosmological model with inhomogeneous space and nonuniform time

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Abstract

A cosmological model with inhomogeneous space and nonuniform time is proposed and substantiated. Both space and time are assumed to be finite, i.e., curved of positive sign and characterized by a variable curvature.

The replacement of the absolute universal time by a relative proper time, intrinsic for individual gravitational objects, is in accord with the spirit of relativity.

Numerous consequences of this model leading to observable phenomena in galaxies, quasars and in the solar system are derived from the mathematical analysis of the line element, Equation (8), of the model in the papers mentioned in Section 4.2, where they are confronted with observational evidence. In addition several predictions following from the theory are listed (Section 4.3), whose verification by future observations may justify the postulate lying at the basis of this theory.

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References

  • Abell, G. O.: 1975, in A. M. Sandage and J. Kristian (eds.),Galaxies and the Universe, University of Chicago Press, Chicago-London, p. 601.

    Google Scholar 

  • Abramenko, B.: 1954,Brit. J. Phil. Sci. 5, 237.

    Google Scholar 

  • Abramenko, B.: 1977,J. Interdiscipl. Cycle Res. 8, 177.

    Google Scholar 

  • Abramenko, B.: 1978a,Astrophys. Space Sci. 54, 323.

    Google Scholar 

  • Abramenko, B.: 1978b, submitted toAstrophys. and Space Sci.

  • Antonov, V. A. and Chernin, A. D.: 1975,Soviet Astron. Lett. 1 121.

    Google Scholar 

  • Baum, W. A.: 1957,Astron. J. 62, 6.

    Google Scholar 

  • Born, M. and Infeld, L.: 1934,Proc. Roy. Soc. A144, 425.

    Google Scholar 

  • De Sitter, W.: 1918,Monthly Notices Roy. Astron. Soc. 78, 3.

    Google Scholar 

  • Dingle, H.: 1934,Monthly Notices Roy. Astron. Soc. 94, 134.

    Google Scholar 

  • Eddington, A. S.: 1925,Relativitätstheorie in mathematischer Behandlung, Springer Verlag, Berlin, p. 246.

    Google Scholar 

  • Einstein, A.: 1917,Sitzber. Preuß. Akad. Wissensch. 1, 142.

    Google Scholar 

  • Einstein, A.: 1950,The Meaning of Relativity (3rd ed.) Princeton University Press, Princeton, N.J., p. 103.

    Google Scholar 

  • Fenelly, A. J.: 1977,Monthly Notices Roy. Astron. Soc. 181, 121.

    Google Scholar 

  • Gott, J. R. III and Thuan, T. X.: 1978,Astrophys. J. 223, 426.

    Google Scholar 

  • Hoyle, F.: 1950,The Nature of the Universe, Blackwell, Oxford, p. 105.

    Google Scholar 

  • Jeans, J.: 1925,Monthly Notices Roy. Astron. Soc. 86, 262.

    Google Scholar 

  • Kiang, T.: 1977,Nature 270 205.

    Google Scholar 

  • Knapp, G. R., Kerr, F. J. and Williams, B. A.: 1978,Astrophys. J. 222, 800.

    Google Scholar 

  • Kristian, J., Sandage, A. and Westphal, J. A.: 1978,Astrophys. J.,221, 383.

    Google Scholar 

  • Lin, D. N. C. and Lynden-Bell, D.: 1977,Monthly Notices Roy. Astron. Soc. 181, 59.

    Google Scholar 

  • Mach, E.: 1912,Die Mechanik in ihrer Entwicklung, 7. ed. Leipzig, p. 217.

  • Mavridis, S.: 1976,Monthly Notices Roy. Astron. Soc. 177, 709.

    Google Scholar 

  • Milne, E.: 1940,Astrophys. J. 91, 129.

    Google Scholar 

  • Noonan, T.: 1971,Publ. Astron. Soc. Pacific 83, 31, 35, 37.

    Google Scholar 

  • Oemler, A. Jr.: 1973,Astrophys. J. 180, 11.

    Google Scholar 

  • Page, Th.: 1975, in A. M. Sandage and J. Kristian (eds.),Galaxies and the Universe, University of Chicago Press, Chicago-London, p. 541.

    Google Scholar 

  • Peach, J. V.: 1970,Astrophys. J. 159, 753.

    Google Scholar 

  • Sandage, A.: 1961a,Astrophys. J. 133, 355.

    Google Scholar 

  • Sandage, A.: 1961b,Astrophys. J. 134, 916.

    Google Scholar 

  • Sandage, A.: 1970,Physics Today 23, No. 2, 34.

    Google Scholar 

  • Sandage, A. and Tammann, G. A.: 1976,Astrophys. J. 210, 7.

    Google Scholar 

  • Seyfert, C.: 1951,Publ. Astron. Soc. Pacific 63, 72.

    Google Scholar 

  • Turner, E. L.: 1976,Astrophys. J. 208, 304.

    Google Scholar 

  • Unsöld, A.: 1947,Z. Astrophysik 24, 278.

    Google Scholar 

  • Van den Bergh, S.: 1977a, in E. M. Berkhuijsen and R. Wielebinski (eds.), Structure and Properties of Nearby Galaxies,IAU Symp. 77, 247.

    Google Scholar 

  • Van den Bergh, S.: 1977b,Vistas Astron. 21, 71.

    Google Scholar 

  • Weinberg, S.: 1972,Gravitation and Cosmology, J. Wiley & Sons, New York, p. 404.

    Google Scholar 

  • Wheeler, J. A.: 1964, in H. Y. Chiu and W. F. Hoffman (eds.),Gravitation and Relativity, Benjamin Inc., New York, Amsterdam, p. 303.

    Google Scholar 

  • Whitrow, G.: 1946,Phil. Mag. (Ser. 7)37, 469.

    Google Scholar 

  • Wolf, R. A. and Bahcall, J. N.: 1972,Astrophys. J. 176, 559.

    Google Scholar 

  • Woltjer, L.: 1971, in D. O'Connell (ed.),Nuclei of Galaxies, Amer. Elsevier Publ. Co., New York, p. 756.

    Google Scholar 

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Abramenko, B. Cosmological model with inhomogeneous space and nonuniform time. Astrophys Space Sci 61, 487–497 (1979). https://doi.org/10.1007/BF00640544

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