Advertisement

The Aporias of Cosmology and the Attempts at Overcoming Them by Nonstandard Models

  • H. Hönl
  • H. Dehnen

Abstract

Of the scientists of modern times Isaac Newton was the first who recognized clearly the cosmological problem and tried to solve it with the help of the general principles of mechanics and of the gravitational law developed by himself. The validity of Euclidean geometry, which includes automatically the spacelike infinity of the Universe, was evident for him as for his forerunners. Herewith, the ground elements of physics and geometry are given, which has been the basis of physics and astronomy up to the beginning of our century.

Keywords

Hyperbolic Space Hubble Parameter Background Radiation Positive Curvature Distance Parameter 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References and Notes

  1. 1.
    S. Hawking and G. Ellis, Astwphys. J. 152, 25 (1968)CrossRefGoogle Scholar
  2. 1a.
    R. Penrose, Phys. Rev. Lett. 14, 57 (1965).CrossRefGoogle Scholar
  3. 2.
    H. Dehnen and H. Hönl, Astwphys. Space Sci. 33, 49 (1975).CrossRefGoogle Scholar
  4. 3.
    P. A. M. Dirac, Nature 139, 323 (1937)CrossRefGoogle Scholar
  5. 3a.
    P. A. M. Dirac, Proc. R. Soc. London Ser. A 165, 199 (1938)CrossRefGoogle Scholar
  6. 3b.
    P. Jordan, Schwerkraft und Weltall (Fr. Vieweg-Verlag, Braunschweig, 1945).Google Scholar
  7. 4.
    F. Hoyle, Mon. Not. R. Astron. Soc. 108, 372 (1948)Google Scholar
  8. 4a.
    H. Bondi and T. Gold, ibid. 108, 252 (1948).Google Scholar
  9. 5.
    H. Hönl and H. Dehnen, Z. Astrophys. 68, 181 (1968)Google Scholar
  10. 5a.
    P. Jordan, ibid. 68, 201 (1968).Google Scholar
  11. 6.
    E. Schrödinger, Physica 6, 899 (1939)CrossRefGoogle Scholar
  12. 6a.
    B. de Witt, Phys. Rev. 90, 357 (1953).Google Scholar
  13. 7.
    H. Urbantke and R. Sexl, Acta Phys. Austriaca 26, 339 (1967).Google Scholar
  14. 8.
    S. G. Mamaev, V. M. Mostepanenko and A. A. Starobinskii, Sov. Phys.-JETP 43, 823 (1976).Google Scholar
  15. 9.
    G. Schäfer and H. Dehnen, J. Phys. A, Math. Gen. 13, 517 (1980).CrossRefGoogle Scholar
  16. 10.
    J. Audretsch, Phys. Lett. 72A, 401 (1979).Google Scholar
  17. 11.
    G. Schäfer and H. Dehnen, Astron. Astrophys. 54, 823 (1977)Google Scholar
  18. 11a.
    G. Schäfer and H. Dehnen, ibid. 61, 671 (1977).Google Scholar
  19. 12.
    E. Schrödinger, Pontifica academia scientiarum, Commentationes 2, 321 (1938).Google Scholar
  20. 13.
    V. N. Lukash and A. A. Starobinskii, Sov. Phys.-JETP 39, 742 (1974).Google Scholar
  21. 14.
    J. E. Gunn and B. M. Tinsley, Nature 257, 454 (1975).CrossRefGoogle Scholar
  22. 15.
    H. Alfvén, Rev. Mod. Phys. 37, 652 (1965)CrossRefGoogle Scholar
  23. 15a.
    R. Omnès, Phys. Rep. 3C, 1 (1972).CrossRefGoogle Scholar

Copyright information

© Plenum Press, New York 1983

Authors and Affiliations

  • H. Hönl
    • 1
  • H. Dehnen
    • 2
  1. 1.Faculty of PhysicsUniversität FreiburgFreiburgGFR
  2. 2.Faculty of PhysicsUniversität KonstanzKonstanzGFR

Personalised recommendations