Quantum gravitational corrected evolution equations of charged black holes

Document Type : Regular article

Author

Bethe Center for Theoretical Physics, University of Bonn, Germany

Abstract

We explain how quantum gravity, treated as an effective field theory, might modify the

evaporative evolution of a four-dimensional, non-extremal, non-rotating, charged black

hole. With some approximations, we derive a set of coupled differential equations describing

the charge and mass of the black hole as a function of time. These equations represent

a generalisation of the analogous ones already present in the literature for classical black

holes.

Keywords

Main Subjects

Journal of Holography Applications in Physics
Volume 3, Issue 1
March 2023
Pages 39-48

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History

  • Receive Date: 10 January 2023
  • Revise Date: 10 February 2023
  • Accept Date: 17 February 2023

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