Holographic microstate counting for AdS$_4$ black holes in massive IIA supergravity
Seyed Morteza Hosseini, Kiril Hristov, Achilleas Passias
TL;DR
This work provides a microscopic holographic account of BPS AdS$_4$ black hole entropy in massive IIA by computing the topologically twisted index of the dual 3d ${\cal N}=2$ CS-matter theories at large $N$ and implementing $\mathcal{I}$-extremization. The authors establish a precise link between the field-theory extremum and the four-dimensional attractor mechanism in the dyonic STU model, including the crucial role of the imaginary part of the partition function. They explicitly analyze the D2$_k$ theory and its AdS$_4\times S^6$ dual, deriving analytic UV and IR geometries and validating the entropy match $\mathcal{I}|_{\rm crit}=S_{\rm BH}$. The results extend the holographic entropy program to a massive IIA setting and illustrate a deep correspondence between horizon data and extremized field-theory indices.
Abstract
We derive the Bekenstein-Hawking entropy for a class of BPS black holes in the massive type IIA supergravity background AdS$_4 \times S^6$ from a microscopic counting of supersymmetric ground states in a holographically dual field theory. The counting is performed by evaluating the topologically twisted index of three-dimensional $\mathcal{N}=2$ Chern-Simons-matter gauge theories in the large $N$ limit. The $\mathcal{I}$-extremization principle is shown to match the attractor mechanism for the near-horizon geometries constructed in the four-dimensional dyonic $\mathcal{N}=2$ gauged supergravity, that arises as a consistent truncation of massive type IIA supergravity on $S^6$. In particular, our results prove that the imaginary part of the three-dimensional partition functions plays a crucial rôle in holography.
