Multicentered black hole saddles for supersymmetric indices

TL;DR

This paper identifies specific finite-temperature supergravity saddle points corresponding to multi-center black holes, providing a gravitational path integral explanation for wall-crossing phenomena in supersymmetric indices.

Contribution

It introduces new saddle points in 4D supergravity that explain how wall-crossing occurs at the level of the gravitational path integral, extending previous Lorentzian analyses.

Findings

Saddles correspond to multi-center black hole contributions to the index.

Wall-crossing is explained by the disappearance of solutions as moduli vary.

Rich moduli space of saddles is analyzed in detail.

Abstract

The supersymmetric index in string theory can sometimes have a discontinuous integer-valued jump at co-dimension one surfaces in moduli space called walls of marginal stability. When the index counts black hole microstates, crossing such walls of marginal stability amounts to the appearance or disappearance of a large number of such states. While wall-crossing has been understood in string theory and through the disappearance of extremal Lorentzian supergravity solutions as the moduli are varied, there has been no understanding about how the discontinuous changes in the index occur at the level of the gravitational path integral. In this paper, we find the finite-temperature saddles in $4d$ flatspace supergravity in which fermionic fields are periodic when going around the thermal circle that correspond to the multi-center black hole contributions to the index. By analyzing these saddles, we can explain how wall-crossing occurs: as the scalar moduli in supergravity are varied at the asymptotic boundary, for a given split of the charges, the saddle point equations can no longer be solved and, consequently, the corresponding multi-center saddle no longer contributes to the index. While the values of the scalars and the jump in the index when a wall is crossed all agree with the prediction from previously found Lorentzian supergravity solutions, the saddles in the index exhibit a much richer moduli space, which we analyze in detail.