Hawking and Page on the brane

@inproceedings{Chamblin2004HawkingAP,
  title={Hawking and Page on the brane},
  author={Andrew Chamblin and Andreas Karch},
  year={2004}
}
.C W e show thatthe H awking-Page phase transition ofa CFT on A dS d (cid:0) 1 weakly coupled to gravity has a dualbulk description in term s ofa phase transition between a black string and a therm algason A dS d .Ateven lowertem peraturestheblack string develops aG regory La(cid:13) am m einstability,which isdualtoblack holeevaporation in theboundary theory. 

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References

SHOWING 1-10 OF 13 REFERENCES

Fate of the black string instability.

This work argues that under very mild assumptions, classical event horizons cannot pinch off and settle down to new static black string solutions which are not translationally invariant along the string.

Black strings and p-branes are unstable.

P perturbations around black strings and branes can be stabilized if the extra dimensions are compactified to a scale smaller than the minimum wavelength for which instability occurs and thus will not affect large astrophysical black holes in four dimensions.

Stable black strings in anti-de Sitter space

In five-dimensional Einstein gravity with a negative cosmological constant in the presence or absence of a non-fine-tuned 3-brane, we investigate the classical stability of black string solutions

The evolution of unstable black holes in anti-de Sitter space

We examine the thermodynamic stability of large black holes in four-dimensional anti-de Sitter space, and we demonstrate numerically that black holes which lack local thermodynamic stability often

Brane world black holes

Gravitational collapse of matter trapped on a brane will produce a black hole on the brane. We discuss such black holes in the models of Randall and Sundrum where our universe is viewed as a domain

An Alternative to compactification

Conventional wisdom states that Newton's force law implies only four noncompact dimensions. We demonstrate that this is not necessarily true in the presence of a nonfactorizable background geometry.

Mass and gauge invariance: Holography for the Karch-Randall model

We argue that the Karch-Randall compactification is holographically dual to a 4D conformal field theory coupled to gravity on anti\char21{}de Sitter space. Using this interpretation we recover the

Quantum Black Holes as Holograms in AdS Braneworlds

We propose a new approach for using the AdS/CFT correspondence to study quantum black hole physics. The black holes on a brane in an AdSD+1 braneworld that solve the classical bulk equations are

Locally localized gravity

We study the fluctuation spectrum of linearized gravity around non-fine-tuned branes. We focus on the case of an AdS4 brane in AdS§. In this case, for small cosmological constant, the warp factor

Exact description of black holes on branes II: comparison with BTZ black holes and black strings

We extend our recent discussion of four-dimensional black holes bound to a two-brane to include a negative cosmological constant on the brane. We find that for large masses, the solutions are