Asymptotically flat rotating topological stars
Abstract We construct a new class of smooth, horizonless, non-supersymmetric solutions in five-dimensional minimal supergravity, which we call rotating topological stars. Built from a Kerr-Taub-bolt geometry embedded in five dimensions, they constitute the first rotating generalization of the topolo...
Tallennettuna:
| Päätekijät: | , , |
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| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
SpringerOpen
2026-03-01
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| Sarja: | Journal of High Energy Physics |
| Aiheet: | |
| Linkit: | https://doi.org/10.1007/JHEP03(2026)108 |
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