English

The spectral form factor in the `t Hooft limit -- Intermediacy versus universality

Strongly Correlated Electrons 2022-09-07 v3 High Energy Physics - Theory Mathematical Physics math.MP

Abstract

The Spectral Form Factor (SFF) is a convenient tool for the characterization of eigenvalue statistics of systems with discrete spectra, and thus serves as a proxy for quantum chaoticity. This work presents an analytical calculation of the SFF of the Chern-Simons Matrix Model (CSMM), which was first introduced to describe the intermediate level statistics of disordered electrons at the mobility edge. The CSMM is characterized by a parameter 0q1 0 \leq q\leq 1, where the Circular Unitary Ensemble (CUE) is recovered for q0q\to 0. The CSMM was later found as a matrix model description of U(N)U(N) Chern-Simons theory on S3S^3, which is dual to a topological string theory characterized by string coupling gs=logqg_s=-\log q. The spectral form factor is proportional to a colored HOMFLY invariant of a (2n,2)(2n,2)-torus link with its two components carrying the fundamental and antifundamental representations, respectively. We check that taking NN \to \infty whilst keeping q<1q<1 reduces the connected SFF to an exact linear ramp of unit slope, confirming the main result from arXiv:2012.11703 for the specific case of the CSMM. We then consider the `t Hooft limit, where NN \to \infty and q1q \to 1^- such that y=qNy = q^N remains finite. As we take q1q\to 1^-, this constitutes the opposite extreme of the CUE limit. In the `t Hooft limit, the connected SFF turns into a remarkable sequence of polynomials which, as far as the authors are aware, have not appeared in the literature thus far. A gap opens in the spectrum and, after unfolding by a constant rescaling, the connected SFF approximates a linear ramp of unit slope for all yy except y1y \approx 1, where the connected SFF goes to zero. We thus find that, although the CSMM was introduced to describe intermediate statistics and the `t Hooft limit is the opposite limit of the CUE, we still recover Wigner-Dyson universality for all yy except y1y\approx 1.

Keywords

Cite

@article{arxiv.2201.07841,
  title  = {The spectral form factor in the `t Hooft limit -- Intermediacy versus universality},
  author = {W. L. Vleeshouwers and V. Gritsev},
  journal= {arXiv preprint arXiv:2201.07841},
  year   = {2022}
}

Comments

Changes: 1. Added a treatment (including plots) of numerically unfolded SFF's for N=10 and N=20 2. Corrected typos 30 pages, 6 figures