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Gravity Waves from Kerr/CFT

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.

preprint2015arXivOpen access
Achilleas P. PorfyriadisAndrew Strominger
astro-ph.HEgr-qchep-th
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Achilleas P. PorfyriadisAndrew Strominger

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