Unitary matrix models, free fermion ensembles, and the giant graviton expansion
Sameer Murthy
TL;DR
The paper develops a unifying framework linking unitary matrix integrals with an infinite set of couplings to free-fermion ensembles, enabling a determinant-based expansion via a Hubbard–Stratonovich transformation. By integrating out fermions and averaging over the auxiliary bosonic variables, the authors derive a convergent $q$-series for the index, with a precise giant-graviton expansion $I^f_N(q)/I^f_\infty(q)=\sum_m G^{(m)}_{f,N}(q)$, where each term is suppressed by $q^{\alpha mN+\alpha m(m+1)/2}$ for a power-series order $\alpha$ of the single-letter index $f(q)$. The main technical tool is the Borodin–Okounkov determinant expansion, recast in a free-fermion language and organized into HS-transformed multi-point kernels; the first nontrivial term ($m=1$) is encoded by a generating function $\widehat K_f(\zeta,q)$ that captures the giant-graviton contributions. The results provide a concrete matrix-model explanation for giant-graviton expansions observed in AdS/CFT contexts and yield explicit formulas for several BPS indices, with numerical checks verifying the predicted order relations and structure.
Abstract
We consider a class of matrix integrals over the unitary group $U(N)$ with an infinite set of couplings characterized by a series $f(q)=\sum_{n \ge 1} a_n q^n$, with $a_n \in \mathbb{Z}$. Such integrals arise in physics as the partition functions of free four-dimensional gauge theories on $S^3$ and, in particular, as the superconformal index of super Yang-Mills theory. We show that any such model can be expressed in terms of a system of free fermions in an ensemble parameterized by the infinite set of couplings. Integrating out the fermions in a given quantum state leads to a convergent expansion as a series of determinants, as shown by Borodin-Okounkov many years ago. By further averaging over the ensemble, we obtain a formula for the matrix integral as a $q$-series with successive terms suppressed by $q^{αN + β}$ where $α$, $β$ do not depend on $N$. This provides a matrix-model explanation of the giant graviton expansion that has been observed recently in the literature.
