Black hole vacua and rotation |
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Authors: | Chethan Krishnan |
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Institution: | SISSA, Via Bonomea 265, 34136, Trieste, Italy |
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Abstract: | Recent developments suggest that the near-region of rotating black holes behaves like a CFT. To understand this better, I propose to study quantum fields in this region. An instructive approach for this might be to put a large black hole in AdS and to think of the entire geometry as a toy model for the “near-region”. Quantum field theory on rotating black holes in AdS can be well-defined (unlike in flat space), if fields are quantized in the co-rotating-with-the-horizon frame. First, some generalities of constructing Hartle–Hawking Green functions in this approach are discussed. Then as a specific example where the details are easy to handle, I turn to 2+1 dimensions (BTZ), write down the Green functions explicitly starting with the co-rotating frame, and observe some structural similarities they have with the Kerr-CFT scattering amplitudes. Finally, in BTZ, there is also an alternate construction for the Green functions: we can start from the covering AdS3 space and use the method of images. Using a 19th century integral formula, I show the equality between the boundary correlators arising via the two constructions. |
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Keywords: | AdS-CFT Black holes QFT in curved space |
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