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Rotational symmetry breaking in baby Skyrme models

2007/10/21 by Itay Hen, Marek Karliner · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Nonlinear Waves and Solitons #Quantum chaos and dynamical systems #hep-th

paper · pdf · doi:10.1088/0951-7715/21/3/002

published as Nonlinearity 21:399-408,2008 · LaTeX, 14 pages, 8 figures

arxiv created 2007/10/21 · openalex publication_date 2008/02/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30

Abstract

We consider multisolitons with charges 1 ⩽ B ⩽ 5 in the baby Skyrme model for the one-parametric family of potentials U = μ 2 (1 − ϕ 3 ) s with 0 < s ⩽ 4. This class of potentials is a generalization of the 'old' ( s = 1) and 'holomorphic' ( s = 4) baby Skyrme models. We find that for charge one, stable solutions exist for every value of s and they are rotationally symmetric. For higher charges, stable solutions exist only below s ≈ 2. In the charge-two sector the stable solutions are always rotationally symmetric and ring-like. For charge three and above, rotational symmetry is exhibited only in the small s region; above a certain critical value of s , this symmetry is broken and a strong repulsion between the constituent one-Skyrmions becomes apparent. We also compute the spatial energy distributions of these solutions.

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