2 v 1 2 6 A pr 1 99 2 Gravitational Lensing and the Variability of G
نویسندگان
چکیده
The four observables associated with gravitational lensing of distant quasars by intervening galaxies: image splittings, relative amplifications, time delays, and optical depths, provide separate measures of the strength of the gravitational constant G at cosmological distances. These allow one, in principle, to factor out unknown lensing parameters to directly to probe the variation of G over cosmological time. We estimate constraints on ˙ G which may be derivable by this method both now and in the future. The limits one may obtain can compete or exceed other direct limits on ˙ G today, but unfortunately extracting this information, is not independent of the effort to fix other cosmological parameters such as H 0 and Ω 0 from lensing observations.
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