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arxiv: hep-th/9808090 · v2 · submitted 1998-08-14 · ✦ hep-th · astro-ph· hep-ph

Vacuum defects without a vacuum

classification ✦ hep-th astro-phhep-ph
keywords defectsmodelsvacuumappreciablearisebreakingdecreasingdensity
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Topological defects can arise in symmetry breaking models where the scalar field potential $V(\phi)$ has no minima and is a monotonically decreasing function of $|\phi|$. The properties of such vacuumless defects are quite different from those of the ``usual'' strings and monopoles. In some models such defects can serve as seeds for structure formation, or produce an appreciable density of mini-black holes.

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  1. Compact structures in impurity-doped vacuumless systems

    hep-th 2026-05 unverdicted novelty 5.0

    Impurities preserving half the BPS sectors induce compact or half-compact stable vacuumless kinks in scalar models, which cannot form in impurity-free canonical cases.