Hawking Radiation from Kerr-Newman Black Hole and Tunneling Mechanism

Abstract

We present the derivation of Hawking radiation by using the tunneling mechanism in a rotating and charged black hole background. We show that the 4-dimensional Kerr-Newman metric, which has a spherically nonsymmetric geometry, becomes an effectively 2-dimensional spherically symmetric metric by using the technique of the dimensional reduction near the horizon. We can thus readily apply the tunneling mechanism to the nonspherical Kerr and Kerr-Newman metric.

18pages, 1 figure

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• Thermal behavior of a radially deformed black hole spacetime
• Hawking Radiation and Tunneling Mechanism for a New Class of Black Holes in Einstein-Gauss-Bonnet Gravity
• Axisymmetric black hole in a non-commutative gauge theory: classical and quantum gravity effects
• Recent Attempts in the Analysis of Black Hole Radiation
• Quasinormal Modes and Hawking Radiation Sparsity of GUP corrected Black Holes in Bumblebee Gravity with Topological Defects
• The black-hole area spectrum in the tunneling formalism with GUP
• Thermodynamics of Black Holes: Semi-Classical Approaches and Beyond