Rotating brane black holes

黑洞在天体物理学和高能物理学中都很重要。然而，当它们与量子场相互作用时，人们对它们的命运知之甚少。理解量子场论在弯曲时空中的行为是一个重要的问题，尤其是因为我们知道宇宙确实包含非常大的曲率区域。虽然在静态（即不旋转）黑洞的背景下取得了一些进展，但对旋转情况（即一般情况）知之甚少。我们希望使用Randall-Sundrum II型模型来解决这个长期存在的问题。这个项目必然涉及在一个大规模的计算平台上求解三维偏微分方程组。

Black holes are important astrophysically and in high energy physics. However, little is known about their fate when they interact with quantum fields. Understanding the behaviour of quantum field theories in curved spacetime is an important problem, not least because we know that the universe does contain regions of very large curvature. While some progress has been made in the context of static (i.e. not rotating) black holes, not much is known about the rotating case (which is the generic case). Using a Randall-Sundrum type II model, we hope to solve this long-standing problem. This project will necessarily involve solving three-dimensional systems of partial differential equations on a large scale computational platform.