Abstract
The coupledDirac-Einstein equations for a homogeneous isotropic space-time forbid aclosed universe but lead to the standard cosmological model for aflat universe. Therefore only theopen universe is left as a nontrivial situation. There some of the desired cosmological effects emerge in a natural way:inflation, creation ex nihilo, etc.
Similar content being viewed by others
References
Blau, S. K., and Guth, A. H. (1987).Inflationary Cosmology, in300 Years of Gravitation, S. W. Hawking and W. Israel, eds., Cambridge University Press, Cambridge.
Lightman, A., and Brawyer, R., eds. (1990).Origins. The Lives and Worlds of Modern Cosmologists, Harvard University Press, New York.
Mattes, M., and Sorg, M. (1991).Zeitschrift für Naturforschung,46a, 967.
Misner, C. W., Thorne, K. S., and Wheeler, J. A. (1973).Gravitation, Freeman, San Francisco.
Penrose, S. (1989). Difficulties with inflationary cosmology, inFourteenth Texas Symposium on Relativistic Astrophysics, E. J. Fenyves, ed., New York.
Rindler, W. (1977).Essential Relativity, Springer, Berlin.
Sorg, M. (1992). Relativistic Schrödinger equations, Preprint, Stuttgart; submitted toZeitschrift für Naturforschung.
Turner, M. (1986). Inflation in the universe, inGeneral Relativity and Gravitation (Proceedings of the 11th International Conference on General Relativity and Gravitation), Stockholm.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Ochs, U., Sorg, M. Fermions and expanding universe. Int J Theor Phys 32, 1531–1547 (1993). https://doi.org/10.1007/BF00672854
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00672854