Hawking Radiation via Higher-spin Gauge Anomalies
Satoshi Iso, Takeshi Morita, Hiroshi Umetsu

TL;DR
This paper extends the anomaly method for deriving Hawking radiation to include higher-spin gauge anomalies, providing a more comprehensive understanding of black hole radiation and its higher moments.
Contribution
It introduces a higher-spin generalization of the anomaly method and trace anomaly approach for Hawking radiation, expanding previous models to include higher moments.
Findings
Derived higher moments of Hawking fluxes using higher-spin anomalies
Generalized the trace anomaly method to higher spins
Connected higher-spin gauge anomalies with black hole radiation
Abstract
We give a higher-spin generalization of the anomaly method for the Hawking radiation from black holes. In the paper arXiv:0710.0453 higher-spin generalizations of the gauge (and gravitational) anomalies in d=2 were obtained. By applying these anomalies to black hole physics, we derive the higher moments of the Hawking fluxes. We also give a higher-spin generalization of the trace anomaly method by Christensen and Fulling.
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