Dynamical vs. Thermodynamical (In)stability of Black Objects in Gravity
By Stefan Hollands (Cardiff U. and Institut für Theoretische Physik, Leipzig)
Understanding the stability properties of black objects is both a very important, but also a
very complex problem in general relativity and its higher dimensional generalizations. Based
on the well-known dictionary between black objects and thermodynamics, it is natural to
come up with criteria for the (in)stability of black objects akin to the standard criteria
involving the ”specific heat” in the context of phenomenological thermodynamics. A key
question is what such notions have to do with notions of instability based on the existence of
”growing modes” of the corresponding perturbed Einstein equations.
In this talk, I review the ”canonical energy method”, which, as I argue, provides a beautiful and clear link between these different concepts of stability (and also a direct connection to the recently proposed approach via a ”local Penrose inequality”). I outline some applications of the canonical energy method, such as a proof of the Gubser-Mitra conjecture for black branes, and a connection between the stability of rotating higher dimensional black holes and that of their associated near horizon geometries, thereby proving a recent conjecture of Durkee-Reall.