Abstract
IN this letter I suggest that the fact that Huygens's principle is not valid in large gravitational fields gives rise to detectable effects.
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
De Witt, B., and De Witt, C., Physics, 1, 145 (1964).
Radhakrishnan, V., and Cooke, D., Astrophys. Lett., 3, 225 (1969).
Croft, M. D., Camella, J. M., and Drake, F. D., Nature, 218, 1122 (1968).
Radhakrishnan, V., Cooke, D. J., Komesaroff, M. M., and Morris, D., Nature, 221, 443 (1969).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
ROE, P. Experimental Method for distinguishing Pulsar Models. Nature 227, 154–156 (1970). https://doi.org/10.1038/227154a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/227154a0
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.