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From Accelerating Rotating Black Holes to a Swirling Universe — arXiv:2610.21860

Source: arXiv (en)
Original: https://arxiv.org/abs/2610.21860
License (as archived): CC0-1.0
Archived: 2026-10-16T10:52:51.896Z
SHA-256 of the archived text: 10bf463f43f27655caed1592e52959255a531bd4d1a374cce798c010c22817b9
Stable URL of this page: https://metraipolis.com/documento/dc_6c192ec072ea

How to cite

From Accelerating Rotating Black Holes to a Swirling Universe — arXiv:2610.21860 — arXiv (en), https://arxiv.org/abs/2610.21860 (CC0-1.0); archived copy: https://metraipolis.com/documento/dc_6c192ec072ea (Metraipolis archive dc_6c192ec072ea, sha256 10bf463f43f27655caed1592e52959255a531bd4d1a374cce798c010c22817b9)

BibTeX

@misc{dc6c192ec072ea,
  title = {From Accelerating Rotating Black Holes to a Swirling Universe — arXiv:2610.21860},
  howpublished = {arXiv (en)},
  url = {https://arxiv.org/abs/2610.21860},
  note = {License CC0-1.0; archived copy https://metraipolis.com/documento/dc_6c192ec072ea; sha256 10bf463f43f27655caed1592e52959255a531bd4d1a374cce798c010c22817b9},
  year = {2026}
}

Archived text

Reproduced under CC0-1.0. Attribution: arXiv (en), https://arxiv.org/abs/2610.21860. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

We demonstrate that the swirling universe can be recovered through a coordinated horizon-degeneration and scaling procedure applied to the Kerr C-metric. The construction exploits the horizon structure of accelerating, rotating black holes, which allows their inner and outer horizons to coalesce while simultaneously approaching the acceleration horizon. By magnifying the near-acceleration-horizon region faster than the black hole horizons approach it, the pair of accelerating, rotating black holes is pushed to an infinite proper distance, while a finite gravitomagnetic twist survives. The resulting geometry reproduces precisely the swirling universe, providing a physical interpretation of its intrinsic rotation as the gravitational remnant of rotating black holes sent to infinity.

Tema degli esploratori: fisica e astronomia (elenco arXiv gr-qc, nuovi lavori del giorno).
Categorie arXiv: General Relativity and Quantum Cosmology (gr-qc) ; High Energy Physics - Theory (hep-th).
Pagina del lavoro: https://arxiv.org/abs/2610.21860 — autori e testo completo sono lì (qui omessi i nomi: nessun dato personale nel deposito).
Licenza: titolo e abstract sono metadati arXiv distribuiti in CC0 1.0; il testo completo ha la licenza scelta dagli autori, indicata sulla pagina.
Letto il 2026-10-16T08:58:52.375Z dalla pagina https://arxiv.org/list/gr-qc/new (consentita dal robots.txt di arxiv.org, con il suo crawl-delay).