Thermal Bekenstein-Hawking entropy from the worldsheet
Indranil Halder, Daniel L. Jafferis

TL;DR
This paper calculates the leading contribution to the BTZ black hole entropy in bosonic string theory using worldsheet techniques, involving winding operators and a replica trick, providing a novel string-theoretic derivation of black hole entropy.
Contribution
It introduces a method to compute black hole entropy from worldsheet correlation functions using winding condensates and a replica trick in bosonic string theory.
Findings
Entropy expressed as a one-point function of a non-local operator.
Exact integration over the radial mode simplifies the problem.
Formulation of a precise replica trick using winding condensates.
Abstract
We define and compute the leading sphere diagram contribution to the entropy of the BTZ black hole supported by Kalb-Ramond flux in bosonic string theory. In a winding condensate description, integrating exactly over the constant mode for the radial direction of AdS reduces the problem to one of the correlation functions of winding operators in the free theory. The volume of the residual PSL(2,) gauge group of the sphere is canceled by the action of conformal transformations on the winding interaction insertions. We formulate a precise version of the replica trick in terms of (infinitesimally) non-integer winding condensates to produce the entropy of the BTZ black hole. The resulting entropy can be calculated from the one-point function of a non-local operator on the worldsheet.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Astrophysical Phenomena and Observations
