Abstract
We show the explicit agreement between the derivation of the Bekenstein–Hawking entropy of a Euclidean BTZ black hole from the point of view of spin foam models and canonical quantization. This is done by considering a graph observable (corresponding to the black hole horizon) in the Turaev–Viro state sum model, and then analytically continuing the resulting partition function to negative values of the cosmological constant.
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Communicated by Carlo Rovelli.
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Geiller, M., Noui, K. BTZ Black Hole Entropy and the Turaev–Viro Model. Ann. Henri Poincaré 16, 609–640 (2015). https://doi.org/10.1007/s00023-014-0331-7
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DOI: https://doi.org/10.1007/s00023-014-0331-7