Gravity Waves from Kerr/CFT
arXiv:1401.3746 · doi:10.1103/PhysRevD.90.044038
Abstract
Dynamics at large redshift near the horizon of an extreme Kerr black hole are governed by an infinite-dimensional conformal symmetry. This symmetry may be exploited to analytically, rather than numerically, compute a variety of potentially observable processes. In this paper we compute and study the conformal transformation properties of the gravitational radiation emitted by an orbiting mass in the large-redshift near-horizon region.
23 pages, v2: reference added, minor changes, matches published version, v3: typos corrected