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We calculate graviton n-point functions in an anti-de Sitter black branebackground for effective gravity theories whose linearized equations of motionhave at most two time derivatives. We compare the n-point functions in Einsteingravity to those in theories whose leading correction is quadratic in theRiemann tensor. The comparison is made for any number of gravitons and for allphysical graviton modes in a kinematic region for which the leading correctioncan significantly modify the Einstein result. We find that the n-pointfunctions of Einstein gravity depend on at most a single angle, whereas thoseof the corrected theories may depend on two angles. For the four-pointfunctions, Einstein gravity exhibits linear dependence on the Mandelstamvariable s versus a quadratic dependence on s for the corrected theory.

Graviton n-point functions for UV-complete theories in Anti-de Sitter space