Abstract
Birkinshaw and Gull1 considered the perturbation of the cosmic background radiation by a moving gravitational lens (GL). An estimate of the maximum amplitude makes it seem possible that this effect may soon be observed, leading to the measurement of non-Hubble velocities of cosmological objects. Such measurements may become a significant test for cosmological models. We present here the general formula for this effect, which differs essentially from that in ref. 1.
Similar content being viewed by others
References
Barkinshaw, M. & Gull, S. F. Nature 302, 315–317 (1983).
Zel'dovich, Ya.B. & Novikov, I. D. The Structure and Evolution of the Universe. (University of Chicago Press, 1983).
Mitrofanov, I. G. Pis'ma Astr. Zh. (Soviet Astr. Lett.) 7, 73–75 (1981).
Collins, C. A., Joseph, R. D. & Robertson, N. A. Nature 320, 506–508 (1986).
Paczynski, B. Nature 319, 567–568 (1986).
Turner, E. L. et al. Nature 321, 142–144 (1986).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Gurvits, L., Mitrofanov, I. Perturbation of the background radiation by a moving gravitational lens. Nature 324, 349–350 (1986). https://doi.org/10.1038/324349a0
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1038/324349a0
- Springer Nature Limited
This article is cited by
-
Diagnostic properties of moving gravitational lenses
Nature (1989)