A cardy formula for three-point coefficients or how the black hole got its spots

Abstract Modular covariance of torus one-point functions constrains the three point function coefficients of a two dimensional CFT. This leads to an asymptotic formula for the average value of light-heavy-heavy three point coefficients, generalizing Cardy’s formula for the high energy density of sta...

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Main Authors: Per Kraus, Alexander Maloney
Format: Article
Language:English
Published: SpringerOpen 2017-05-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP05(2017)160
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author Per Kraus
Alexander Maloney
author_facet Per Kraus
Alexander Maloney
author_sort Per Kraus
collection DOAJ
description Abstract Modular covariance of torus one-point functions constrains the three point function coefficients of a two dimensional CFT. This leads to an asymptotic formula for the average value of light-heavy-heavy three point coefficients, generalizing Cardy’s formula for the high energy density of states. The derivation uses certain asymptotic properties of one-point conformal blocks on the torus. Our asymptotic formula matches a dual AdS3 computation of one point functions in a black hole background. This is evidence that the BTZ black hole geometry emerges upon course-graining over a suitable family of heavy microstates.
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spelling doaj.art-2684686348f2456190e7a0f8063118f12022-12-22T00:05:10ZengSpringerOpenJournal of High Energy Physics1029-84792017-05-012017512210.1007/JHEP05(2017)160A cardy formula for three-point coefficients or how the black hole got its spotsPer Kraus0Alexander Maloney1Department of Physics and Astronomy, University of CaliforniaPhysics Department, McGill UniversityAbstract Modular covariance of torus one-point functions constrains the three point function coefficients of a two dimensional CFT. This leads to an asymptotic formula for the average value of light-heavy-heavy three point coefficients, generalizing Cardy’s formula for the high energy density of states. The derivation uses certain asymptotic properties of one-point conformal blocks on the torus. Our asymptotic formula matches a dual AdS3 computation of one point functions in a black hole background. This is evidence that the BTZ black hole geometry emerges upon course-graining over a suitable family of heavy microstates.http://link.springer.com/article/10.1007/JHEP05(2017)160AdS-CFT CorrespondenceConformal Field TheoryBlack Holes in String TheoryGauge-gravity correspondence
spellingShingle Per Kraus
Alexander Maloney
A cardy formula for three-point coefficients or how the black hole got its spots
Journal of High Energy Physics
AdS-CFT Correspondence
Conformal Field Theory
Black Holes in String Theory
Gauge-gravity correspondence
title A cardy formula for three-point coefficients or how the black hole got its spots
title_full A cardy formula for three-point coefficients or how the black hole got its spots
title_fullStr A cardy formula for three-point coefficients or how the black hole got its spots
title_full_unstemmed A cardy formula for three-point coefficients or how the black hole got its spots
title_short A cardy formula for three-point coefficients or how the black hole got its spots
title_sort cardy formula for three point coefficients or how the black hole got its spots
topic AdS-CFT Correspondence
Conformal Field Theory
Black Holes in String Theory
Gauge-gravity correspondence
url http://link.springer.com/article/10.1007/JHEP05(2017)160
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