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Stability of topological solitons, and black string to bubble transition

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arxiv 2112.11474 v2 pith:G4Y3LIAO submitted 2021-12-21 hep-th gr-qchep-ph

classification hep-thgr-qchep-ph
keywords blacksolitonsstringslocally-stableobjectstopologicalactionboundary
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abstract

We study the existence of smooth topological solitons and black strings as locally-stable saddles of the Euclidean gravitational action of five dimensional Einstein-Maxwell theory. These objects live in the Kaluza-Klein background of four dimensional Minkowski with an $S^1$. We compute the off-shell gravitational action in the canonical ensemble with fixed boundary data corresponding to the asymptotic radius of $S^1$, and to the electric and magnetic charges that label the solitons and black strings. We show that these objects are locally-stable in large sectors of the phase space with varying lifetime. Furthermore, we determine the globally-stable phases for different regimes of the boundary data, and show that there can be Hawking-Page transitions between the locally-stable phases of the topological solitons and black strings. This analysis demonstrates the existence of a large family of globally-stable smooth solitonic objects in gravity beyond supersymmetry, and presents a mechanism through which they can arise from the black strings.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit

    gr-qc 2025-06 conditional novelty 6.0 of 10

    For Topological Stars, the eikonal-limit renormalized angular momentum is expressed as hypergeometric functions tied to the null geodesic radial action, generalizing the Schwarzschild resummation.

  2. Nonradial stability of topological stars

    gr-qc 2025-02 conditional novelty 6.0 of 10

    Numerical linear perturbation analysis finds no instability in nonradial Type-II modes of topological stars with zero Kaluza-Klein momentum.

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