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Stringy Horizons and UV/IR Mixing
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abstract
The target-space interpretation of the exact (in $\alpha'$) reflection coefficient for scattering from Euclidean black-hole horizons in classical string theory is studied. For concreteness, we focus on the solvable $SL(2, \mathbb{R})_k/U(1)$ black hole. It is shown that it exhibits a fascinating UV/IR mixing, dramatically modifying the late-time behavior of general relativity. We speculate that this might play an important role in the black-hole information puzzle, as well as in clarifying features related with the non-locality of Little String Theory.
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Cited by 1 Pith paper
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Stringy Black Hole Interiors
The paper argues that the operator F, the fusion of winding string operators W+ and W-, describes folded strings that fill the SL(2,R)/U(1) black hole and radiate at the Hawking temperature.
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