PIRSA:14050009

Gravity waves from Kerr/CFT

Porfyriadis, A. (2014). Gravity waves from Kerr/CFT. Perimeter Institute. https://pirsa.org/14050009

Porfyriadis, Achilleas. Gravity waves from Kerr/CFT. Perimeter Institute, May. 15, 2014, https://pirsa.org/14050009 

          @misc{ pirsa_PIRSA:14050009,
            doi = {10.48660/14050009},
            url = {https://pirsa.org/14050009},
            author = {Porfyriadis, Achilleas},
            keywords = {Strong Gravity},
            language = {en},
            title = {Gravity waves from Kerr/CFT},
            publisher = {Perimeter Institute},
            year = {2014},
            month = {may},
            note = {PIRSA:14050009 see, \url{https://pirsa.org}}
          }

Achilleas Porfyriadis

Harvard University

Talk number
PIRSA:14050009
Collection
Talk Type
Subject
Abstract
Astronomical observation suggests the existence of near-extreme Kerr black holes whose horizons spin at nearly the speed of light. Properties of diffeomorphisms imply that the dynamics of the high-redshift near-horizon region of near-extreme Kerr, which includes the innermost-stable-circular-orbit (ISCO), is governed by an infinite-dimensional emergent conformal symmetry. This symmetry may be exploited to analytically, rather than numerically, compute a variety of potentially observable processes. In this talk I will show how we compute and study the conformal transformation properties of the gravitational radiation emitted by an orbiting massive object in the large-redshift near-horizon region. I will also use conformal symmetry of the near-horizon region to compute the gravitational radiation produced during the plunge phase following the object's crossing of the ISCO.