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arXiv · 2006.09681

Hawking radiation particle spectrum of a Kerr-Newman black hole

Joshua Foo·Michael R. R. Good
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Abstract

Charged, rotating Kerr-Newman black holes represent the most general class of asymptotically flat black hole solutions to the Einstein-Maxwell equations of general relativity. Here, we consider a simplified model for the Hawking radiation produced by a Kerr-Newman black hole by utilising a (1+1)-dimensional accelerated boundary correspondence (i.e. a flat spacetime mirror trajectory) in Minkowski spacetime. We derive the particle spectrum and its late-time thermal distribution which reduces to the Kerr, Reissner-Nordstr\"om and Schwarzschild cases in the appropriate limits. We also compute the particle spectrum of the extremal Kerr-Newman system and the total energy emitted.

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Joshua Foo, Michael R. R. Good. 2020-06-17. Hawking radiation particle spectrum of a Kerr-Newman black hole. https://doi.org/10.1088/1475-7516/2021/01/019

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