On vacuum gravitational collapse in nine dimensions
P. Bizoń, T. Chmaj, A. Rostworowski, B. G. Schmidt, Z. Tabor
Abstract
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.
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