It turns out that repulsive effect due to rotation of a rotating black hole dominates over attraction due to mass for large $r$ in dimensions $>5$. This gives rise to a remarkable result that black hole in these higher dimensions in contrast to lower dimensional ones cannot be overspun even under linear test particle accretion. Further if a black hole in dimension $>4$ has one of its rotation parameters zero, it has only one horizon and hence it can never be overspun. Thus rotating black holes in six and higher dimensions, and those with one rotation parameter switched off, would always obey the weak cosmic censorship conjecture (WCCC).

中文翻译：

---

在较大尺寸的黑洞上过度旋转

事实证明，由于旋转黑洞的旋转而产生的排斥作用在质量引起的吸引力上占主导地位 $\mathrm{[R}$ 在尺寸上 $>5$。这产生了显着的结果，即使在线性测试颗粒堆积的情况下，与较低维的黑洞相比，这些较高维的黑洞也不能过度旋转。此外，如果尺寸上有黑洞$>4$旋转参数之一为零，视野只有一个，因此永远不能过分旋转。因此，在六个或更高维度上旋转黑洞，并关闭一个旋转参数的黑洞将始终服从弱宇宙检查猜想（WCCC）。