Perturbation of the background radiation by a moving gravitational lens

Mathematics – Logic

Scientific paper

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Scientific paper

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.

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