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arXiv · 1401.3746

Gravity Waves from Kerr/CFT

Achilleas P. Porfyriadis·Andrew Strominger
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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.

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Achilleas P. Porfyriadis, Andrew Strominger. 2015-05-30. Gravity Waves from Kerr/CFT. https://doi.org/10.1103/physrevd.90.044038

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