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Solitons in relativistic field theories are not necessarily topologically charged. In particular, non-topological solitons – known as Q-balls – arise naturally in nonlinear field theories endowed with attractive interactions and internal symmetries. Even without stabilizing internal symmetries, quasi-solitons known as oscillons, which are long-lived, can also exist. Both Q-balls and oscillons have significant applications in cosmology and particle physics. This review is an updated account of the intriguing properties and dynamics of these non-topological solitons and quasi-solitons, as well as their important roles in early-universe scenarios and particle physics models.

生成讲解博客的中文版本

生成AI智能校验的中文版本