Back Reaction from Trace Anomaly in RN-blackholes Evaporation

Details Back Reaction from Trace Anomaly in RN-blackholes Evaporation Back Reaction from Trace Anomaly in RN-blackholes Evaporation

2004-02-03

arxiv.org/abs/gr-qc/0402017v1

JHEP 0312:055,2003

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages Latex

Scientific paper

10.1088/1126-6708/2003/12/055

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.

Affiliated with

Also associated with

No associations

Rating

Back Reaction from Trace Anomaly in RN-blackholes Evaporation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Back Reaction from Trace Anomaly in RN-blackholes Evaporation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Back Reaction from Trace Anomaly in RN-blackholes Evaporation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-565216