Hawking Radiation in a Plebanski-Demianski Black Hole
arXiv:1211.6685 · doi:10.1007/JHEP06(2013)001
Abstract
In this paper, we show the flux of Hawking radiation in a Plebański-Demiański black hole from the point of view of gauge and gravitational anomalies. We will use the consistent anomaly method to guarantee that our results are valid in the de Sitter space. This is because we are including the cosmological constant into our parameters and the covariant anomaly method gives a wrong value for the Hawking temperature. We also show that these calculations are a general result. In order to verify the consistence of our results, we can reproduce earlier known results as certain limiting cases.
19 page
References in corpus (11)
- Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies
- Hawking radiation from rotating black holes in anti-de Sitter spaces via gauge and gravitational anomalies
- Comments on anomaly versus WKB/tunneling methods for calculating Unruh radiation
- Quantum Anomalies at Horizon and Hawking Radiations in Myers-Perry Black Holes
- Gravitational Anomalies, Hawking Radiation, and Spherically Symmetric Black Holes
- Hawking radiation from black holes in de Sitter spaces
- Gravitational anomalies: a recipe for Hawking radiation
- Hawking radiation, W-infinity algebra and trace anomalies
- Hawking Fluxes, Algebra and Anomalies
- Higher-spin Gauge and Trace Anomalies in Two-dimensional Backgrounds
- Hawking radiation, chirality, and the principle of effective theory of gravity