Table of Contents
Fetching ...

A tale of two cascades: Higgsing and Seiberg-duality cascades from type IIB string theory

Eduardo Conde, Jerome Gaillard, Carlos Nunez, Maurizio Piai, Alfonso V. Ramallo

TL;DR

This work constructs explicit type IIB supergravity solutions with brane sources that dualize to N=1 field theories featuring a Seiberg-duality cascade in the UV and a finite-range Higgsing cascade in the intermediate regime, culminating in IR confinement with a smooth end of space. By starting from a wrapped-D5 system and applying a solution-generating rotation, the authors obtain UV-complete backgrounds connected to KS/BGMPZ, with a controllable distribution of flavor sources encoded by a profile S(ρ). They analyze two classes of solutions (exact and semi-analytic), study the resulting field-theory dynamics, compute holographic central charges, and propose UV-tail profiles to tame the high-energy behavior, highlighting potential applications to dynamical electroweak symmetry breaking and tumbling-like dynamics in strongly coupled gauge theories.

Abstract

We construct explicitly new solutions of type IIB supergravity with brane sources, the duals of which are N = 1 supersymmetric field theories exhibiting two very interesting phenomena. The far UV dynamics is controlled by a cascade of Seiberg dualities analogous to the Klebanov- Strassler backgrounds. At intermediate scales a cascade of Higgsing appears, in the sense that the gauge group undergoes a sequence of spontaneous symmetry breaking steps which reduces its rank. Deep in the IR, the theory confines, and the gravity background has a non-singular end of space. We explain in detail how to generate such solutions, discuss some of the Physics associated with them and briefly comment on the possible applications.

A tale of two cascades: Higgsing and Seiberg-duality cascades from type IIB string theory

TL;DR

This work constructs explicit type IIB supergravity solutions with brane sources that dualize to N=1 field theories featuring a Seiberg-duality cascade in the UV and a finite-range Higgsing cascade in the intermediate regime, culminating in IR confinement with a smooth end of space. By starting from a wrapped-D5 system and applying a solution-generating rotation, the authors obtain UV-complete backgrounds connected to KS/BGMPZ, with a controllable distribution of flavor sources encoded by a profile S(ρ). They analyze two classes of solutions (exact and semi-analytic), study the resulting field-theory dynamics, compute holographic central charges, and propose UV-tail profiles to tame the high-energy behavior, highlighting potential applications to dynamical electroweak symmetry breaking and tumbling-like dynamics in strongly coupled gauge theories.

Abstract

We construct explicitly new solutions of type IIB supergravity with brane sources, the duals of which are N = 1 supersymmetric field theories exhibiting two very interesting phenomena. The far UV dynamics is controlled by a cascade of Seiberg dualities analogous to the Klebanov- Strassler backgrounds. At intermediate scales a cascade of Higgsing appears, in the sense that the gauge group undergoes a sequence of spontaneous symmetry breaking steps which reduces its rank. Deep in the IR, the theory confines, and the gravity background has a non-singular end of space. We explain in detail how to generate such solutions, discuss some of the Physics associated with them and briefly comment on the possible applications.

Paper Structure

This paper contains 29 sections, 98 equations, 7 figures.

Figures (7)

  • Figure 1: We plot an example of a possible D5-brane configuration: a total of $N_f$ D5s extend in the radial coordinate from some minimum $\rho$, that can lie between $\rho_*$ and $\rho_{**}$, to infinity. We chose a distribution of minimal radial distances of the D5s that is homogeneous in $\rho$, as indicated by the dotted oblique line. This configuration of D5s gives rise to the plotted $S(\rho)$, which is asymptotically constant ($S(\rho)\rightarrow1$).
  • Figure 2: After the rotation, D3-brane charge is induced on the D5s. As argued in Section \ref{['twokinds']}, this charge grows exponentially with the radial distance. An asymptotically constant profile $S(\rho)$ will generate an infinite amount D3-brane charge.
  • Figure 3: Plot of the profile function (\ref{['vvvvzzzz']}). The function $S(\rho)$ starts growing for small $\rho$, reaches a maximum, and then decreases exponentially for large values of the holographic coordinate.
  • Figure 4: For the case $N_c = N_f =2$ and $h_1 = 5$, we show the functions defining the semi-analytic rotated background. The choice of $S(\rho)$ is the one specified in the text (eq. (\ref{['vvvvzzzz']})).
  • Figure 5: Plots of the function $c(\rho)$ for $N_c = N_f =2$ and $h_1 = 5$. We considered the backgrounds of Section \ref{['semianalyticdetails']}.
  • ...and 2 more figures