On vacuum gravitational collapse in nine dimensions
  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. 
P. Bizo\'n, T. Chmaj, A. Rostworowski, B. G. Schmidt, Z. Tabor