  It has been recently observed that a scalar field with Robin boundary
conditions (RBCs) can trigger both a superradiant and a bulk instability for a
BTZ black hole (BH). To understand the generality and scrutinize the origin of
this behavior, we consider here the superradiant instability of a Kerr BH
confined either in a mirror-like cavity or in AdS space, triggered also by a
scalar field with RBCs. These boundary conditions are the most general ones
that ensure the cavity/AdS space is an isolated system, and include, as a
particular case, the commonly considered Dirichlet boundary conditions (DBCs).
Whereas the superradiant modes for some RBCs differ only mildly from the ones
with DBCs, in both cases we find that as we vary the RBCs, the imaginary part
of the frequency may attain arbitrarily large positive values. We interpret
this growth as being sourced by a bulk instability of both confined geometries
when certain RBCs are imposed to either the mirror-like cavity or the AdS
boundary, rather than by energy extraction from the BH, in analogy with the BTZ
behavior.
