Quantum black holes and holography
release_4vcrzclqczazbfrgysowyld3da
by
Alessandro Fabbri
2005
Abstract
It is technically difficult (if not impossible) to write down and solve
self-consistently the semiclassical Einstein equations in the case of
evaporating black holes. These difficulties can in principle be overcome in an
apparently very different context, the Randall-Sundrum braneworld models in
Anti-de Sitter space. Use of Maldacena's AdS/CFT correspondence led us to
formulate a holographic conjecture for black holes localised on a brane, for
which 4D quantum corrected black holes are dual to classical 5D black holes.
This duality is applied to the computation of the correction to the newtonian
potential on the brane, with new results on the semiclassical side, and a
prediction about the existence of static large mass braneworld black holes is
made.
In text/plain
format
Archived Content
There are no accessible files associated with this release. You could check other releases for this work for an accessible version.
Know of a fulltext copy of on the public web? Submit a URL and we will archive it
hep-th/0512180v1
access all versions, variants, and formats of this works (eg, pre-prints)