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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
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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

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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