English

Stokes Phenomena and Non-perturbative Completion in the Multi-cut Two-matrix Models

High Energy Physics - Theory 2011-09-28 v3 Mathematical Physics math.MP

Abstract

The Stokes multipliers in the matrix models are invariants in the string-theory moduli space and related to the D-instanton chemical potentials. They not only represent non-perturbative information but also play an important role in connecting various perturbative string theories in the moduli space. They are a key concept to the non-perturbative completion of string theory and also expected to imply some remnant of strong coupling dynamics in M theory. In this paper, we investigate the non-perturbative completion problem consisting of two constraints on the Stokes multipliers. As the first constraint, Stokes phenomena which realize the multi-cut geometry are studied in the Z_k symmetric critical points of the multi-cut two-matrix models. Sequence of solutions to the constraints are obtained in general k-cut critical points. A discrete set of solutions and a continuum set of solutions are explicitly shown, and they can be classified by several constrained configurations of the Young diagram. As the second constraint, we discuss non-perturbative stability of backgrounds in terms of the Riemann-Hilbert problem. In particular, our procedure in the 2-cut (1,2) case (pure-supergravity case) completely fixes the D-instanton chemical potentials and results in the Hastings-McLeod solution to the Painlev\'e II equation. It is also stressed that the Riemann-Hilbert approach realizes an off-shell background independent formulation of non-critical string theory.

Keywords

Cite

@article{arxiv.1011.5745,
  title  = {Stokes Phenomena and Non-perturbative Completion in the Multi-cut Two-matrix Models},
  author = {Chuan-Tsung Chan and Hirotaka Irie and Chi-Hsien Yeh},
  journal= {arXiv preprint arXiv:1011.5745},
  year   = {2011}
}

Comments

71 pages, v3: organization of Sec. 3, Sec. 4, App. C and App. D improved, final version to be published in Nucl. Phys. B

R2 v1 2026-06-21T16:49:16.322Z