Abstract
Abstract While tested to a high level of accuracy in
the Solar system, general relativity is under the spotlight of both
theoreticians and observers on larger scales, mainly because of the
need to introduce dark matter and dark energy in the cosmological
model. This text reviews the main tests of general relativity focusing
on the large scale structure and more particularly weak lensing.
The complementarity with other tests (including those on Solar system
scales and the equivalence principle) is discussed.
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