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Effective theories and black hole production in warped compactifications
High Energy Physics - Theory · Submitted 22 Sep 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Breakdown of the effective description occurs when either five-dimensional physics or strong gravity becomes important.
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The abstract, sentence by sentence
We investigate aspects of the four-dimensional effective description of brane world scenarios based on warped compactification on anti-de Sitter space. The low-energy dynamics is described by visible matter gravitationally coupled to a ``dark'' conformal field theory. We give the linearized description of the 4d stress tensor corresponding to an arbitrary 5d matter distribution. In particular a 5d falling particle corresponds to a 4d expanding shell, giving a 4d interpretation of a trajectory that misses a black hole only by moving in the fifth dimension. Breakdown of the effective description occurs when either five-dimensional physics or strong gravity becomes important. In scenarios with a TeV brane, the latter can happen through production of black holes near the TeV scale. This could provide an interesting experimental window on quantum black hole dynamics.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We investigate aspects of the four-dimensional effective description of brane world scenarios based on warped compactification on anti-de Sitter space. | contribution 0.79 | 0.78 | 0.05 | asserted 0.86 |
| s1 | The low-energy dynamics is described by visible matter gravitationally coupled to a ``dark'' conformal field theory. | background 0.79 | 0.25 | 0.07 | asserted 1.00 |
| s2 | We give the linearized description of the 4d stress tensor corresponding to an arbitrary 5d matter distribution. | contribution 0.88 | 0.90 | 0.07 | asserted 1.00 |
| s3 | In particular a 5d falling particle corresponds to a 4d expanding shell, giving a 4d interpretation of a trajectory that misses a black hole only by moving in the fifth dimension. | interpretation 0.74 | 0.77 | 0.24 | asserted 1.00 |
| s4 | Breakdown of the effective description occurs when either five-dimensional physics or strong gravity becomes important. | limitation 0.90 | 0.52 | 0.22 | asserted 1.00 |
| s5 | In scenarios with a TeV brane, the latter can happen through production of black holes near the TeV scale. | interpretation 0.78 | 0.17 | 0.18 | hedged possibility 0.54 |
| s6 | This could provide an interesting experimental window on quantum black hole dynamics. | interpretation 0.98 | 0.07 | 0.15 | hedged possibility 1.00 |
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Original abstract
We investigate aspects of the four-dimensional effective description of brane world scenarios based on warped compactification on anti-de Sitter space. The low-energy dynamics is described by visible matter gravitationally coupled to a ``dark'' conformal field theory. We give the linearized description of the 4d stress tensor corresponding to an arbitrary 5d matter distribution. In particular a 5d falling particle corresponds to a 4d expanding shell, giving a 4d interpretation of a trajectory that misses a black hole only by moving in the fifth dimension. Breakdown of the effective description occurs when either five-dimensional physics or strong gravity becomes important. In scenarios with a TeV brane, the latter can happen through production of black holes near the TeV scale. This could provide an interesting experimental window on quantum black hole dynamics.
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References
How the literature uses it
10 arXiv papers cite this in 11 sentences
Papers citing it · 7 sentences without a confident label
Cites it as background 4 papers
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The idea was first explored in the non-compact Randall-Sundrum model[Usually called RS2, to distinguish it from original RS model, also called RS1.] [ref] (some examples can be found in Refs. [ref] ).
Dark Matter Phenomenology: Sterile Neutrino Portal and Gravitational Portal in Extra-Dimensions · AdS/CFT Correspondence and RS Model · 0.83
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Early discussions of this in large extra dimension scenarios and warped scenarios are [ref] respectively.
High-energy black hole production · Introduction · 0.88
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The localization phenomenon has been interpreted in the context of AdS/CFT [ref] , by the observation that the RSII model in a $d+1$-dimensional AdS bulk (and its curved-brane descendents in $d+1$-dimensional AAdS spacetimes) should be equivalent to a $d$-dimensional CFT with some UV cutoff coupled to dynamical gravity on the brane.[This doesn't provide a full microscopic description of the theory since the dynamical gravity is added in “by hand” to the cutoff CFT.
Black Hole Microstate Cosmology · Gravity localization in the Randall-Sundrum II model · 0.80
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