Circular Wilson loops in defect ${\cal N}$=4 SYM: phase transitions, double-scaling limits and OPE expansion
S. Bonansea (Florence U.), S. Davoli (Parma U.), L. Griguolo (Parma, U.), D. Seminara (Florence U.)

TL;DR
This paper investigates phase transitions and operator expansions of circular Wilson loops in a defect $ ext{N}=4$ SYM theory, revealing different behaviors for BPS and non-BPS cases at strong coupling and large flux.
Contribution
It provides a detailed analysis of Wilson loop phase transitions, double-scaling limits, and OPE expansions in a defect $ ext{N}=4$ SYM, highlighting differences between BPS and non-BPS configurations.
Findings
Non-BPS loops exhibit a Gross-Ooguri-like phase transition.
BPS loops lack cylindrical solutions, indicating saturation by supergravity modes.
The double-scaling limit is consistent for non-BPS loops but fails for BPS loops.
Abstract
We consider circular Wilson loops in a defect version of super-Yang-Mills theory which is dual to the D3-D5 brane system with units of flux. When the loops are parallel to the defect, we can construct both BPS and non-BPS operators, depending on the orientation of the scalar couplings in the R-symmetry directions. At strong 't Hooft coupling we observe, in the non supersymmetric case, a Gross-Ooguri-like phase transition in the dual gravitational theory: the familiar disk solution dominates, as expected, when the operator is far from the defect while a cylindrical string worldsheet, connecting the boundary loop with the probe D5-brane, is favourite below a certain distance (or equivalently for large radii of the circles). In the BPS case, instead, the cylindrical solution does not exist for any choice of the physical parameters, suggesting that the exchange of light…
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