Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-26T09:34:52.972Z Has data issue: false hasContentIssue false
  • English
  • Français

Gravitation and cosmic expansion in conformal space-time

Published online by Cambridge University Press:  24 October 2008

Feza Gürsey  and
H. Bondi
Feza Gürsey
Affiliation:
Physics DepartmentUniversity of Istanbul
Get access Rights & Permissions [Opens in a new window]

Abstract

A simple theory of gravitation is formulated in conformal Riemannian space-time. The metric is determined by a scalar function which satisfies a linear equation. A conclusion in favour of Einstein's general tensor theory is drawn from a discussion of the corrections to the Newtonian theory for purely gravitational phenomena. Finally the theory is applied to the cosmological problem and especially to the possibility of a steady-state universe. The velocity-distance law is shown to be compatible with a constant uniform distribution of matter without the need of artificial assumptions.

Type
Research Article
Information
Mathematical Proceedings of the Cambridge Philosophical Society , Volume 49 , Issue 2 , April 1953 , pp. 285 - 291
Copyright
Copyright © Cambridge Philosophical Society 1953

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

(1)Einstein, A.The meaning of relativity, 4th ed. (London, 1950).Google Scholar
(2)Eisenhart, L. P.Riemannian geometry (Princeton, 1926).Google Scholar
(3)Hoyle, F.Mon. Not. R. astr. Soc. 108 (1948), 372.CrossRefGoogle Scholar
(4)Infeld, L. and Schild, A.Phys. Rev. (2), 68 (1945), 250.CrossRefGoogle Scholar
(5)Infeld, L. and Schild, A.Phys. Rev. (2), 70 (1946), 410.CrossRefGoogle Scholar
(6)Mccrea, W. H.Proc. roy. Soc. A, 206 (1951), 562.Google Scholar
(7)Nordström, G.Ann. Phys., Lpz., 40 (1913), 856.CrossRefGoogle Scholar
(8)Nordström, G.Ann. Phys., Lpz., 42 (1913), 533.CrossRefGoogle Scholar