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We give a higher-spin generalization of the anomaly method for the Hawking radiation from black holes.
S. Hawking, “Black Hole Explosions,” Nature (London) 248
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To an observer outside a black hole, gravity in the near-horizon region has two-dimensional conformal symmetries. This fact is stressed in the following references; S. Carlip, “Black hole entropy from conformal field theory in any dimension,” Phys. Rev. Lett. 82
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R. Bertlmann, Anomalies in Quantum Field Theory
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K. Fujikawa and H. Suzuki, Path integrals, and quantum anomalies
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S. P. Robinson and F. Wilczek, “A relationship between Hawking radiation and gravitational anomalies,” Phys. Rev. Lett. 95
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S. Iso, H. Umetsu and F. Wilczek, “Hawking radiation from charged black holes via gauge and gravitational anomalies,” Phys. Rev. Lett. 96
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S. Iso, H. Umetsu and F. Wilczek, “Anomalies, Hawking radiations and regularity in rotating black holes,” Phys. Rev. D 74
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K. Murata and J. Soda, “Hawking radiation from rotating black holes and gravitational anomalies,” Phys. Rev. D 74
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S. Iso, T. Morita and H. Umetsu, “Quantum anomalies at horizon and Hawking radiations in Myers-Perry black holes,” JHEP 0704
2007
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E. C. Vagenas and S. Das, JHEP 0610
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S. Iso, T. Morita and H. Umetsu, “Higher-spin currents and thermal flux from Hawking radiation,” Phys. Rev. D 75
2007
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2007
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