Hawking Radiation via Gauss-Bonnet Theorem
arXiv:1902.04465 · doi:10.1016/j.aop.2020.168071
Abstract
In this paper, we apply the topological method to the various black holes to derive their Hawking temperature. We show that the this method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology. Therefore, we conclude that the topological method provides a consistent formula to achieve the Hawking temperature.
5 pages. Version accepted for publication in Annals of Physics
References in corpus (14)
- Tunnelling, Temperature and Taub-NUT Black Holes
- An exact Schwarzschild-like solution in a bumblebee gravity model
- Subtleties in the quasi-classical calculation of Hawking radiation
- The GUP effect on Hawking Radiation of the 2+1 dimensional Black Hole
- Tunneling of Vector Particles from Lorentzian Wormholes in 3+1 Dimensions
- Black hole radiation of spin-1 particles in (1+2) dimensions
- Uninformed Hawking Radiation
- Hawking Radiation via Tunneling from Hot NUT-Kerr-Newman-Kasuya Spacetime
- The Effect of the Gauss-Bonnet term to Hawking Radiation from arbitrary dimensional Black Brane
- On Holographic Dual of the Dyonic Reissner-Nordström Black Hole
- Hawking radiation of linear dilaton black holes
- Quasinormal Modes of a Schwarzschild Black Hole Immersed in an Electromagnetic Universe
- On the Topological Nature of the Hawking Temperature of Black Holes
- Global Hawking Temperature of Schwarzschild-de Sitter Spacetime: a Topological Approach