Allowable complex metrics and the gravitational index of AdS$_5$ black holes
Pietro Benetti Genolini, Oliver Janssen, Sameer Murthy
TL;DR
The paper analyzes the Kontsevich–Segal–Witten criterion for the allowability of complex metrics in the gravitational path integral describing the supersymmetric index of AdS$_5$ black holes with two angular momenta. It develops an eigenvalue-based algorithm to test KSW stability and demonstrates that, at the conformal boundary, the KSW conditions are equivalent to the microscopic convergence constraints on the BPS trace; extending this into the bulk via the Fefferman–Graham expansion and numerical study shows that the KSW constraints do not enlarge the allowed region beyond the microscopic one. The authors prove that BKSW coincides with the microscopic region and provide strong numerical evidence that the full KSW criterion, when applied to these complex AdS$_5$ saddles, yields the same allowed region as the microscopic index, i.e., $ extsf{KSW}= extsf{micro}$. This builds on prior results in AdS and flat space and clarifies the interplay between gravitational allowability and microscopic convergence for a holographic supersymmetric index. The work also offers a practical computational approach for implementing KSW in holographic contexts and highlights the tension between boundary and bulk conditions in complex geometries.
Abstract
We discuss the Kontsevich-Segal-Witten criterion for the allowability of complex metrics, in the context of the gravitational path integral that calculates the supersymmetric index. We focus on the saddle points that capture the contribution of supersymmetric black holes in AdS$_5$ space. We show that, for such black holes with two independent angular momenta, the conditions imposed on the corresponding saddle point by the KSW criterion are equivalent to the ones arising from the convergence of the microscopic trace form of the supersymmetric index. This result adds to previous results establishing such an equivalence in other, simpler examples of the gravitational index in AdS space and flat space. Along the way, we give a practical algorithm for implementing the KSW criterion in terms of eigenvalues of certain matrices.
