Renormalization Group Flow, Stability, and Bulk Viscosity in a Large N Thermal QCD Model
arXiv:1611.07998 · doi:10.1103/PhysRevD.95.086018
Abstract
The ultraviolet completion of a large N QCD model requires introducing new degrees of freedom at certain scale so that the UV behavior may become asymptotically conformal with no Landau poles and no UV divergences of Wilson loops. These UV degrees of freedom are represented by certain anti-branes arranged on the blown-up sphere of a warped resolved conifold in a way that they are separated from the other set of branes that control the IR behavior of the theory. This separation of the branes and the anti-branes creates instability in the theory. Further complications arise from the curvature of the ambient space. We show that, despite these analytical hurdles, stability may still be achieved by switching on appropriate world-volume fluxes on the branes. The UV degrees of freedom, on the other hand, modify the RG flow in the model. We discuss this in details by evaluating the flow from IR confining to UV conformal. Finally we lay down a calculational scheme to study bulk viscosity which, in turn, would signal the inherent non-conformality in this model.
49 pages, 8 figures; v2: Section 4.4 expanded and the bulk viscosity computations made more precise, typos corrected and figure 4 replaced by its sharper image. Final version to appear in Physical Review D
References in corpus (12)
- Viscosity in Strongly Interacting Quantum Field Theories from Black Hole Physics
- Schwinger-Keldysh Propagators from AdS/CFT Correspondence
- Exploring improved holographic theories for QCD: Part II
- Effect of curvature squared corrections in AdS on the viscosity of the dual gauge theory
- Deconfinement and Gluon Plasma Dynamics in Improved Holographic QCD
- Exotic RG Flows from Holography
- Heavy Quarkonium Melting in Large N Thermal QCD
- UV-divergences of Wilson Loops for Gauge/Gravity Duality
- Holography with a Landau pole
- A UV complete model of Large N Thermal QCD
- Heavy Quark Potential at Finite Temperature in a Dual Gravity Closer to Large N QCD
- Backreaction effects due to matter coupled higher derivative gravity