Abstract
KAFKA1 has considered the possibility that gravitational radiation is of primordial origin. He treated this radiation in the high frequency limit2 and used the Friedmann equations to determine its effect on the evolution of the cosmos. Using Weber's intensity measurements, he found that the lifetime of the universe would be shortened to 3.3 × 109 yr and concluded that the observed wave pulses cannot be remnants of the big bang.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Kafka, P., Nature, 226, 436 (1970).
Isaacson, R. A., Phys. Rev., 166, 1263 (1968).
Weber, J., Sci. Amer., 224, 22 (1971).
Braginskii, V. B., Zel'dovich, Ya. B., and Rudenko, V. N., Sov. Phys. JETP Lett., 10, 280 (1969).
Gibbons, G. W., and Hawking, S. W., Phys. Rev., D 4, 2191 (1971).
Dicke, R. H., Astrophys. J., 155, 123 (1969).
Iben, I., and Faulkner, J., Astrophys. J., 153, 101 (1968).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
ISAACSON, R., WINICOUR, J. Cosmic Effects of Gravitational Waves. Nature 239, 447–448 (1972). https://doi.org/10.1038/239447a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/239447a0
This article is cited by
-
A maximal background spectrum of gravitational radiation
Astrophysics and Space Science (1976)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.