Hawking fluxes and Anomalies in Rotating Regular Black Holes with a Time-Delay

Understand

Based on the anomaly cancellation method we are going to compute the Hawking fluxes (the Hawking thermal flux and the total flux of energy-momentum tensor) from a four-dimensional rotating regular black hole with a time-delay.

• To this purpose, in the three metrics proposed in arXiv:1510.08828, we try to perform the dimensional reduction in which the anomaly cancellation method is feasible at the near-horizon region in a general scalar field theory.
• As a result we can demonstrate that the dimensional reduction is possible in two of those metrics.
• Hence we perform the anomaly cancellation method and compute the Hawking fluxes in those two metrics.