Non-Abelian k-Vortex Dynamics in N=1^* theory and its Gravity Dual
Roberto Auzzi, S. Prem Kumar

TL;DR
This paper investigates non-Abelian k-vortex solutions in N=1^* theory, demonstrating their properties, tensions, and dual descriptions, revealing Casimir scaling and connections to string theory via the gravity dual.
Contribution
It provides explicit non-Abelian vortex solutions in N=1^* theory and matches their tensions with string dual descriptions, highlighting Casimir scaling and the role of the gravity dual.
Findings
k-vortex tensions follow Casimir scaling law
World-sheet theta angle matches semiclassical predictions
Dual D-brane configurations realize vortex solutions
Abstract
We study magnetic flux tubes in the Higgs vacuum of the N=1^* mass deformation of SU(N_c), N=4 SYM and its large N_c string dual, the Polchinski-Strassler geometry. Choosing equal masses for the three adjoint chiral multiplets, for all N_c we identify a "colour-flavour locked" symmetry, SO(3)_{C+F} which leaves the Higgs vacuum invariant. At weak coupling, we find explicit non-Abelian k-vortex solutions carrying a Z_{N_c}-valued magnetic flux, with winding, 0 < k < N_c. These k-strings spontaneously break SO(3)_{C+F} to U(1)_{C+F} resulting in an S^2 moduli space of solutions. The world-sheet sigma model is a nonsupersymmetric CP^1 model with a theta angle \theta_{1+1} = k(N_c-k)\theta_{3+1} where \theta_{3+1} is the Yang-Mills vacuum angle. We find numerically that k-vortex tensions follow the Casimir scaling law T_k \propto k (N_c-k) for large N_c. In the large N_c IIB string dual,…
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