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Spontaneous breaking of baryon symmetry in strongly coupled three-dimensional theories

Antón F. Faedo, Carlos Hoyos, Javier G. Subils

TL;DR

This work shows that baryon-number symmetry $U(1)_{\mathcal B}$ is spontaneously broken in a class of ${\cal N}=1$ $2+1$-dimensional theories with a discrete spectrum by constructing and analyzing a Goldstone-mode vector fluctuation in a holographic dual. Through a consistent four-dimensional supergravity truncation containing a massless vector dual to the monopole current and a baryonic vector, the authors derive the full set of coupled vector equations and implement a Goldstone-mode ansatz. They solve the equations in both confining ($k=0$) and non-confining ($k\neq 0$) backgrounds, using analytic reductions and numerical shooting to demonstrate normalizable, regular solutions that correspond to the Goldstone mode, with the mode persisting even when a nonzero Chern–Simons level is present. The results reinforce the holographic picture of a baryonic sector akin to the Klebanov–Strassler cascade in lower dimensions and motivate further checks via baryon-operator vevs and potential moduli-space structure.

Abstract

We show that baryon number symmetry is spontaneously broken in a class of three-dimensional, ${\cal N}=1$ supersymmetric theories with a discrete mass spectrum. These models serve as lower-dimensional, less-supersymmetric analogs of the Klebanov-Strassler solution, sharing properties such as the presence of a cascade. The spontaneous symmetry breaking is evidenced by the appearance of a Goldstone mode, which corresponds to a vector fluctuation in the gravity dual.

Spontaneous breaking of baryon symmetry in strongly coupled three-dimensional theories

TL;DR

This work shows that baryon-number symmetry is spontaneously broken in a class of -dimensional theories with a discrete spectrum by constructing and analyzing a Goldstone-mode vector fluctuation in a holographic dual. Through a consistent four-dimensional supergravity truncation containing a massless vector dual to the monopole current and a baryonic vector, the authors derive the full set of coupled vector equations and implement a Goldstone-mode ansatz. They solve the equations in both confining () and non-confining () backgrounds, using analytic reductions and numerical shooting to demonstrate normalizable, regular solutions that correspond to the Goldstone mode, with the mode persisting even when a nonzero Chern–Simons level is present. The results reinforce the holographic picture of a baryonic sector akin to the Klebanov–Strassler cascade in lower dimensions and motivate further checks via baryon-operator vevs and potential moduli-space structure.

Abstract

We show that baryon number symmetry is spontaneously broken in a class of three-dimensional, supersymmetric theories with a discrete mass spectrum. These models serve as lower-dimensional, less-supersymmetric analogs of the Klebanov-Strassler solution, sharing properties such as the presence of a cascade. The spontaneous symmetry breaking is evidenced by the appearance of a Goldstone mode, which corresponds to a vector fluctuation in the gravity dual.

Paper Structure

This paper contains 13 sections, 44 equations, 2 figures.

Figures (2)

  • Figure 1: Left: numerical solution for $\hat{\alpha}$ (blue) and $\tilde{\alpha}$ (red) that interpolates smoothly between the two asymptotic regimes \ref{['eq:expasions_conf_UV']}, \ref{['eq:expasions_conf_IR']}. The boundary is located at $\rho_0/\rho\to0$. Right: corresponding profile for $\mathcal{A}$ as given by \ref{['eq:A1_profile']}.
  • Figure 2: Left: numerical solution for $\gamma_+$ (black) and $\beta$ (orange) that interpolates smoothly between the two asymptotic regimes \ref{['eq:expasions_B8_UV']} and \ref{['eq:expasions_B8_IR']}. Right: corresponding profile of $\mathcal{A}$.