2005/11/12 by Piotr Bizoń, P. Bizoń, Tadeusz Chmaj +7
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Pulsars and Gravitational Waves Research #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.72.121502
published as Phys.Rev. D72 (2005) 121502 · 4 pages, 4 figures
arxiv created 2005/11/12 · openalex publication_date 2005/12/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01
We consider the vacuum gravitational collapse for cohomogeneity-two solutions of the nine dimensional Einstein equations. Using combined numerical and analytical methods we give evidence that within this model the Schwarzschild-Tangherlini black hole is asymptotically stable. In addition, we briefly discuss the critical behavior at the threshold of black-hole formation.