Classical Black Hole Evaporation in Randall-Sundrum Infinite Braneworld

By Takahiro Tanaka. 2002

161 citations recorded by the source corpus.

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.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/4ba020657352600ac5ed78c97fac8ac71ca4ff12

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Nuclear and High Energy Physics

Citations in the corpus

Quantum Black Holes as Holograms in AdS Braneworlds (2002, unknown): “Tanaka [35], and, simultaneously, by R.”
Ricci solitons, Ricci flow and strongly coupled CFT in the Schwarzschild Unruh or Boulware vacua (2011, background): “We note that this is very much related to the issue of existence of RandallSundrum braneworld static black holes [13,28–33], where we believe the arguments against their existence based on extrapolation from free field theory would also incorrectly imply non-existence of the solution we have found h”
Spherical black holes with regular center: a review of existing models including a recent realization with Gaussian sources (2008, unknown): “those about brane-world black holes [126, 23, 75, 127].”
Modified Gravity and Cosmology (2011, background): “When applied to the problem of finding a black hole on the brane, this suggests that the solution should not be static since it should include the back-reaction of the Hawking radiation [470] (see also [1201]).”
Brane-World Gravity (2004, background): “Using N ∼ l(2)/G, this gives an evaporation timescale [406] tevap ∼ (︂ M M⊙ )︂3(︂ 1 mm l )︂2 yr.”
Massive islands (2020, background): “[31, 32] were the first to point out that by the standard rules of AdS/CFT quantum effects, including the Hawking radiation, on the RS brane should be encoded in the classical bulk geometry.”
Static axisymmetric vacuum solutions and non-uniform black strings (2002, background): “One exciting avenue for future research is to understand how to include localised horizons in the scheme, which would allow access to uncharged black hole solutions in Kaluza-Klein theory, and on branes, if the latter solutions do indeed exist, (although the converse has recently been conjectured by”