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Analysis

This paper addresses inconsistencies in previous calculations of extremal and non-extremal three-point functions involving semiclassical probes in the context of holography. It clarifies the roles of wavefunctions and moduli averaging, resolving discrepancies between supergravity and CFT calculations for extremal correlators, particularly those involving giant gravitons. The paper proposes a new ansatz for giant graviton wavefunctions that aligns with large N limits of certain correlators in N=4 SYM.
Reference

The paper clarifies the roles of wavefunctions and averaging over moduli, concluding that holographic computations may be performed with or without averaging.