论文标题
exp时间黑孔
Black Holes at Exp-time
论文作者
论文摘要
古典GR长期以来控制着黑洞的演变，但在某些呈指数型的时间里，它必须崩溃。崩溃以及之后的内容尚未得到很好的理解。在本文中，我将使用从复杂性几何形状提取的概念讨论问题。特别是，切割基因座的几何概念起着关键作用。
Classical GR governs the evolution of black holes for a long time, but at some exponentially large time it must break down. The breakdown, and what comes after it, is not well understood. In this paper I'll discuss the problem using concepts drawn from complexity geometry. In particular the geometric concept of cut locus plays a key role.
