English

Back Reaction from Trace Anomaly in RN-blackholes Evaporation

General Relativity and Quantum Cosmology 2010-01-15 v1

Abstract

A model is proposed to describe a transition from a charged black hole of mass MM and charge QQ to one of mass Mˉ\bar{M} and charge Qˉ\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.

Keywords

Cite

@article{arxiv.gr-qc/0402017,
  title  = {Back Reaction from Trace Anomaly in RN-blackholes Evaporation},
  author = {Fabrizio Canfora and Gaetano Vilasi},
  journal= {arXiv preprint arXiv:gr-qc/0402017},
  year   = {2010}
}

Comments

16 pages Latex