Hostname: page-component-77c89778f8-n9wrp Total loading time: 0 Render date: 2024-07-16T11:37:06.175Z Has data issue: false hasContentIssue false
  • English
  • Français

A New Test of the Theory of General Relativity

Published online by Cambridge University Press:  25 April 2016

D. F. Crawford
D. F. Crawford*
Affiliation:
School of Physics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

It has been recently suggested (Crawford 1979) that there is an interaction between a photon and curved space-time that can be observed as a redshift of the photon frequency. Since the amount of the redshift is a function of the curvature it may be used to discriminate between gravitational theories. This is easily done using the parametrized post-Newtonian (PPN) limit fully described in the review article by Will (1972).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 5 , 1979 , pp. 364
Copyright
Copyright © Astronomical Society of Australia 1979

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

Crawford, D.F., Nature, ITI, 633 (1979).CrossRefGoogle Scholar
Goldstein, R.M., Science, 166, 598 (1969).Google Scholar
Merat, P., Pecker, J.-C, and Vigier, J.-P., Astr. Astrophys. 30, 167 (1974).Google Scholar
Will, CM., (1973) in Experimental Gravitation, Proceedings of the International School of Physics ‘Enrico Fermi’ Course 56, ed. Bertotti, B. (Academic Press: New York).Google Scholar