Finite-gap equations for strings on AdS_3 x S^3 x T^4 with mixed 3-form flux
Andrei Babichenko, Amit Dekel, Olof Ohlsson Sax
TL;DR
The paper advances integrability methods for string theory on $AdS_3 \times S^3 \times T^4$ with mixed RR and NSNS flux by deriving finite-gap equations from a generalized $\mathbb{Z}_4$-symmetric Lax framework and connecting them to an all-loop Bethe ansatz built from the Hoare--Tseytlin S-matrix. It shows that in the thermodynamic limit the Bethe equations reproduce the finite-gap construction while also providing leading-order and one-loop corrections to the dressing phases, and it analyzes semiclassical spectra through BMN quantization and classical solutions such as circular strings and giant magnons, including finite-size effects. The results extend the standard AdS/CFT integrability toolkit to backgrounds with mixed flux, enabling non-perturbative insights and cross-checks via S-duality; they also pave the way for incorporating massless modes and applying to other AdS$_3$ backgrounds. Overall, the work synthesizes algebraic-curve, Bethe-ansatz, and semiclassical analyses to yield a coherent picture of the classical and semi-classical spectrum in mixed-flux AdS$_3$ string theory, with precise predictions for dressing phases and finite-size corrections.
Abstract
We study superstrings on AdS_3 x S^3 x T^4 supported by a combination of Ramond-Ramond and Neveu-Schwarz-Neveu-Schwarz three form fluxes, and construct a set of finite-gap equations that describe the classical string spectrum. Using the recently proposed all-loop S-matrix we write down the all-loop Bethe ansatz equations for the massive sector. In the thermodynamic limit the Bethe ansatz reproduces the finite-gap equations. As part of this derivation we propose expressions for the leading order dressing phases. These phases differ from the well-known Arutyunov-Frolov-Staudacher phase that appears in the pure Ramond-Ramond case. We also consider the one-loop quantization of the algebraic curve and determine the one-loop corrections to the dressing phases. Finally we consider some classical string solutions including finite size giant magnons and circular strings.
