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PreprintCC BY 4.0arXiv

Multi-Boundary Spinning AdS5 Black Holes, Strongly Coupled Plasma Balls and a dual locally de Sitter spacetime

Abstract

We construct a new family of exact spinning black hole solutions in five-dimensional General Relativity with a negative cosmological constant, which are dual to strongly coupled spinning plasma balls on four-dimensional Minkowski spacetime. In analogy with the recent discovery of such black solutions in four bulk dimensions, the boundary Lorentz factor acts as a new coordinate in the bulk, giving rise to a new UV region that, in our case, is locally a three-dimensional de Sitter spacetime times the real line. The dual energy-momentum tensor in this region describes a conformal anisotropic fluid that satisfies the weak and strong energy conditions.

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BibTeX
@misc{anabalon2026multiboundary,
  title = {{Multi-Boundary Spinning $AdS_5$ Black Holes, Strongly Coupled Plasma Balls and a dual locally de Sitter spacetime}},
  author = {Andrés Anabalón and Guillermo Buckle and Annelies Fullgraff and Marcelo Oyarzo},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.22084},
  eprint = {2609.22084},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.22084},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Multi-Boundary Spinning AdS_5 Black Holes, Strongly Coupled Plasma Balls and a dual locally de Sitter spacetime
AU  - Andrés Anabalón
AU  - Guillermo Buckle
AU  - Annelies Fullgraff
AU  - Marcelo Oyarzo
PY  - 2026
DA  - 2026/09/18
PB  - arXiv
DO  - 10.48550/arxiv.2609.22084
UR  - https://arxiv.org/abs/2609.22084
AB  - We construct a new family of exact spinning black hole solutions in five-dimensional General Relativity with a negative cosmological constant, which are dual to strongly coupled spinning plasma balls on four-dimensional Minkowski spacetime. In analogy with the recent discovery of such black solutions in four bulk dimensions, the boundary Lorentz factor acts as a new coordinate in the bulk, giving rise to a new UV region that, in our case, is locally a three-dimensional de Sitter spacetime times the real line. The dual energy-momentum tensor in this region describes a conformal anisotropic fluid that satisfies the weak and strong energy conditions.
ER  -