PIRSA:16110029

Video URL

https://pirsa.org/16110029

Gravitational waves via Kerr/CFT

Hadar, S. (2016). Gravitational waves via Kerr/CFT. Perimeter Institute for Theoretical Physics. https://pirsa.org/16110029

Hadar, Shahar. Gravitational waves via Kerr/CFT. Perimeter Institute for Theoretical Physics, Nov. 17, 2016, https://pirsa.org/16110029 

          @misc{ scivideos_PIRSA:16110029,
            doi = {10.48660/16110029},
            url = {https://pirsa.org/16110029},
            author = {Hadar, Shahar},
            keywords = {Strong Gravity},
            language = {en},
            title = {Gravitational waves via Kerr/CFT},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2016},
            month = {nov},
            note = {PIRSA:16110029 see, \url{https://scivideos.org/index.php/pirsa/16110029}}
          }

Shahar Hadar Harvard University

Talk numberPIRSA:16110029
DOI10.48660/16110029
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Massive objects orbiting a near-extreme Kerr black hole plunge into the horizon after passing the innermost stable circular orbit, producing a potentially observable signal of gravitational radiation. The near horizon dynamics of such rapidly rotating black holes is governed by a conformal symmetry. In the talk I will show how this symmetry can be exploited to analytically compute the gravitational waves produced by a variety of orbits. I will also discuss an application to gravitational self-force and comment on the holographic interpretation of the process.