PIRSA:06010002

Video URL

https://pirsa.org/06010002

The universality of highly damped quasinormal modes in generic single horizon black holes

Daghigh, R. (2006). The universality of highly damped quasinormal modes in generic single horizon black holes. Perimeter Institute for Theoretical Physics. https://pirsa.org/06010002

Daghigh, Ramin. The universality of highly damped quasinormal modes in generic single horizon black holes. Perimeter Institute for Theoretical Physics, Jan. 12, 2006, https://pirsa.org/06010002 

          @misc{ scivideos_PIRSA:06010002,
            doi = {10.48660/06010002},
            url = {https://pirsa.org/06010002},
            author = {Daghigh, Ramin},
            keywords = {Quantum Gravity},
            language = {en},
            title = {The universality of highly damped quasinormal modes in generic single horizon black holes},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2006},
            month = {jan},
            note = {PIRSA:06010002 see, \url{https://scivideos.org/pirsa/06010002}}
          }

Ramin Daghigh

Talk numberPIRSA:06010002
DOI10.48660/06010002
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

We calculate analytically the highly damped quasinormal mode spectra of generic single-horizon black holes using the rigorous WKB techniques of Andersson and Howls. We thereby provide a firm foundation for previous analysis, and point out some of their possible limitations. The numerical coefficient in the real part of the highly damped frequency is generically determined by the behavior of coupling of the perturbation to the gravitational field near the origin, as expressed in tortoise coordinates. This fact makes it difficult to understand how the (in)famous ln(3) could be related to the quantum gravitational microstates near the horizon.