Kerr-Newman-Taub-NUT Black Hole Tunnelling Radiation
arXiv:1808.01020 · doi:10.1140/epjp/s13360-023-04605-x
Abstract
The tunnelling process always occur nearby the event horizon of the black hole. In this paper, we investigate the tunnelling radiation in the background of the Kerr-Newman-Taub-NUT black hole. The new coordinate system for Kerr-Newman-Taub-NUT is introduced, which helps us to form new line element. This line element helps us to show that new coordinate is exhaustively acted at event horizon. With the help of conservation of angular momentum, self gravitational effect and energy, we will show that Hawking's radiation is not exclusively thermal.
arXiv comment14 pages, 15 figures
References in corpus (11)
- Hawking Radiation as Tunneling
- Photon Regions and Shadows of Kerr-Newman-NUT Black Holes with a Cosmological Constant
- A Secret Tunnel Through The Horizon
- Hawking radiation as tunneling from the Kerr and Kerr-Newman black holes
- Radiation via Tunneling from a de Sitter Cosmological Horizon
- Hawking Radiation from AdS Black Holes
- How the Change in Horizon Area Drives Black Hole Evaporation
- Gravitomagnetism in the Kerr-Newman-Taub-NUT spacetime
- Hawking radiation as tunneling derived from Black Hole Thermodynamics through the quantum horizon
- Center of Mass Energy of the Collision for Two General Geodesic Particles Around a Kerr-Newman-Taub-NUT Black Hole
- Probing Gravitational Interactions of Elementary Particles