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Gravitational induction

Published online by Cambridge University Press:  24 October 2008

H. Levy
H. Levy
Affiliation:
University of Surrey
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Abstract

Near-field transfer of gravitational energy for quasi-static axisymmetric systems is investigated by a perturbation method; a relativistic analogue of Bondi's Newtonian Poynting vector is defined. It is concluded that a quasi-static axisymmetric system can lose energy only in the presence of a receiver.

Type
Research Article
Information
Mathematical Proceedings of the Cambridge Philosophical Society , Volume 64 , Issue 4 , October 1968 , pp. 1081 - 1087
Copyright
Copyright © Cambridge Philosophical Society 1968

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References

REFERENCES

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(5)Synge, J. L.Relativity, the general theory, ch. 8. (1960).Google Scholar