Bulk Dynamics in Confining Gauge Theories
Marcus Berg, Michael Haack, Wolfgang Muck
TL;DR
The work develops a gauge-invariant, sigma-model–covariant framework for bulk fluctuations in a 5D fake-supergravity truncation of type IIB supergravity, enabling controlled analysis of confining gauge theories. Applying the method to MN and KS backgrounds, the authors derive and solve fluctuation equations, obtaining explicit glueball spectra for MN and analytic, UV-focused solutions for KS in the moderate-UV regime, with careful discussion of boundary conditions and singularities. These results demonstrate the feasibility of handling generally coupled scalar bulk fluctuations and provide a concrete step toward computing correlators in confining gauge theories via holography, while highlighting the dictionary and renormalization challenges that remain in non-AdS settings. The framework offers practical tools for probing UV and IR dynamics, operator mixing, and the role of non-perturbative condensates in holographic duals of confining gauge theories.
Abstract
We consider gauge/string duality (in the supergravity approximation) for confining gauge theories. The system under scrutiny is a 5-dimensional consistent truncation of type IIB supergravity obtained using the Papadopoulos-Tseytlin ansatz with boundary momentum added. We develop a gauge-invariant and sigma-model-covariant approach to the dynamics of 5-dimensional bulk fluctuations. For the Maldacena-Nunez subsystem, we study glueball mass spectra. For the Klebanov-Strassler subsystem, we compute the linearized equations of motion for the 7-scalar system, and show that a 3-scalar sector containing the scalar dual to the gluino bilinear decouples in the UV. We solve the fluctuation equations exactly in the "moderate UV" approximation and check this approximation numerically. Our results demonstrate the feasibility of analyzing the generally coupled equations for scalar bulk fluctuations, and constitute a step on the way towards computing correlators in confining gauge theories.
