Classical black hole evaporation in Randall-Sundrum infinite braneworld

Details Classical black hole evaporation in Randall-Sundrum infinite braneworld Classical black hole evaporation in Randall-Sundrum infinite braneworld

2002-03-24

arxiv.org/abs/gr-qc/0203082v2

Prog.Theor.Phys.Suppl.148:307-316,2003

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Style file changed, Proceedings for YITP workshop "Braneworld -Dynamics of spacetime boundary"

Scientific paper

10.1143/PTPS.148.307

After the gravity induced on the brane in the Randall-Sundrum (RS) infinite braneworld is briefly reviewed, we discuss the possibility that black holes evaporate as a result of classical evolution in this model based on the AdS/CFT correspondence. If this possibility is really the case, the existence of long-lived solar mass black holes will give the strongest constraint on the bulk curvature radius. At the same time, we can propose a new method to simulate the evaporation of a 4D black hole due to the Hawking radiation as a 5D process.

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