Finite temperature corrections to black hole quasinormal modes from 2D CFT

Abstract We revisit the holographic calculation of the decay modes of the BTZ blackhole perturbed by a scalar probe. We carry out a finite temperature expansion of the torus two point function of large central charge (c) CFTs in order to obtain the corrections to blackhole quasinormal modes. We take...

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Main Author: Sanchari Pal
Format: Article
Language:English
Published: SpringerOpen 2022-08-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP08(2022)150
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author Sanchari Pal
author_facet Sanchari Pal
author_sort Sanchari Pal
collection DOAJ
description Abstract We revisit the holographic calculation of the decay modes of the BTZ blackhole perturbed by a scalar probe. We carry out a finite temperature expansion of the torus two point function of large central charge (c) CFTs in order to obtain the corrections to blackhole quasinormal modes. We take the contribution of the lightest primary above the vacuum, with dimension ∆ χ and upper bound of c/6, in the torus two point function. We exploit the modular properties of 2D CFT on the torus to connect the expression of thermal two point function at high temperature with the same at low temperature. The correction term can be expressed as a four point function on the Riemann sphere. In the dual bulk theory the corrections are expected to arise due to the presence of a light matter field in the spacetime along with gravity. In the holographic limit the effects of this correction term is encoded in the change in blackhole temperature. This leads to new quasinormal modes and modification of thermalization time scale.
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spelling doaj.art-f54dfdeb85ad48f9af379aa0c1aab45d2022-12-22T01:37:18ZengSpringerOpenJournal of High Energy Physics1029-84792022-08-012022811910.1007/JHEP08(2022)150Finite temperature corrections to black hole quasinormal modes from 2D CFTSanchari Pal0Department of Physics, Indian Institute of Technology — KanpurAbstract We revisit the holographic calculation of the decay modes of the BTZ blackhole perturbed by a scalar probe. We carry out a finite temperature expansion of the torus two point function of large central charge (c) CFTs in order to obtain the corrections to blackhole quasinormal modes. We take the contribution of the lightest primary above the vacuum, with dimension ∆ χ and upper bound of c/6, in the torus two point function. We exploit the modular properties of 2D CFT on the torus to connect the expression of thermal two point function at high temperature with the same at low temperature. The correction term can be expressed as a four point function on the Riemann sphere. In the dual bulk theory the corrections are expected to arise due to the presence of a light matter field in the spacetime along with gravity. In the holographic limit the effects of this correction term is encoded in the change in blackhole temperature. This leads to new quasinormal modes and modification of thermalization time scale.https://doi.org/10.1007/JHEP08(2022)150AdS-CFT CorrespondenceBlack Holes
spellingShingle Sanchari Pal
Finite temperature corrections to black hole quasinormal modes from 2D CFT
Journal of High Energy Physics
AdS-CFT Correspondence
Black Holes
title Finite temperature corrections to black hole quasinormal modes from 2D CFT
title_full Finite temperature corrections to black hole quasinormal modes from 2D CFT
title_fullStr Finite temperature corrections to black hole quasinormal modes from 2D CFT
title_full_unstemmed Finite temperature corrections to black hole quasinormal modes from 2D CFT
title_short Finite temperature corrections to black hole quasinormal modes from 2D CFT
title_sort finite temperature corrections to black hole quasinormal modes from 2d cft
topic AdS-CFT Correspondence
Black Holes
url https://doi.org/10.1007/JHEP08(2022)150
work_keys_str_mv AT sancharipal finitetemperaturecorrectionstoblackholequasinormalmodesfrom2dcft