Back Reaction from Trace Anomaly in RN-blackholes Evaporation

Abstract

A model is proposed to describe a transition from a charged black hole of mass $M$ and charge $Q$ to one of mass $\bar{M}$ and charge $\bar{Q}$. The basic equations are derived from the non-vacuum Einstein field equations sourced by the Coulomb field and by a null scalar field with a nonvanishing trace anomaly. It is shown that the nonvanishing trace of the energy-momentum tensor prevents the formation of a naked singularity.

16 pages Latex

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Cited by in corpus (3)

• Analogue Gravity
• Influence of the back reaction of the Hawking radiation upon black hole quasinormal modes
• Incompressible fluid inside an astrophysical black hole?