Abstract
RECENTLY Woodward and Yourgrau1 put forward the hypothesis that the influence of gravitation on the propagation of electromagnetic waves depends on the frequency of the radiation. Their starting point is that the light deflexion by the Sun's gravitational field, as found from optical determinations at solar eclipses, appears somewhat larger2,3 than the value predicted by Einstein's theory of gravitation. Lately Muhleman et al.4 and Seielstad et al.5 succeeded in measuring the light deflexion by the Sun at 2.388 GHz and 9.602 GHz. Their results (1.82″ ± 0.2″ and 1.77″ ± 0.2 ″) are in close agreement with the predictions of general relativity. The uncertainty introduced by our limited knowledge of the coronal plasma amounts to about 10 per cent of the relativistic light deflexion4, which, being sufficient to prevent a decision between Einstein's theory and the Brans-Dicke theory, is not enough to make these measurements compatible with the predictions of Woodward and Yourgrau. Their hypothesis (according to formula (2), or (1) and (3))1 gives at 2.388 GHz and 9.602 GHz the tremendous values of 15′ 39″ and 7′ 45″ respectively for the light deflexion (that is, more than 500 times and 200 times the experimental results).
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.