  Extremal scalar three-point correlators in the near-NHEK geometry of Kerr
black holes have recently been shown to agree with the result expected from a
holographically dual non-chiral two-dimensional conformal field theory. In this
paper we extend this calculation to extremal three-point functions of scalars
in a general Kerr black hole which need not obey the extremality condition
$M=\sqrt{J}$. It was recently argued that for low frequency scalars in the Kerr
geometry there is a dual conformal field theory description which determines
the interactions in this regime. Our results support this conjecture.
Furthermore, we formulate a recipe for calculating finite-temperature retarded
three-point correlation functions which is applicable to a large class of (even
non-extremal) correlators, and discuss the vanishing of the extremal couplings.
