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A Note on Warped String Compactification
High Energy Physics - Theory · Submitted 26 Mar 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We give a short review of a large class of warped string geometries, obtained via F-theory compactified on Calabi-Yau fourfolds, that upon reduction to 5 dimensions give consistent supersymmetric realizations of the RS compactification scenario.
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We give a short review of a large class of warped string geometries, obtained via F-theory compactified on Calabi-Yau fourfolds, that upon reduction to 5 dimensions give consistent supersymmetric realizations of the RS compactification scenario.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We give a short review of a large class of warped string geometries, obtained via F-theory compactified on Calabi-Yau fourfolds, that upon reduction to 5 dimensions give consistent supersymmetric realizations of the RS compactification scenario. | contribution 0.99 | 0.43 | 0.46 | asserted 0.99 |
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Original abstract
We give a short review of a large class of warped string geometries, obtained via F-theory compactified on Calabi-Yau fourfolds, that upon reduction to 5 dimensions give consistent supersymmetric realizations of the RS compactification scenario.
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References
How the literature uses it
14 arXiv papers cite this in 15 sentences
Papers citing it · 8 sentences without a confident label
Builds on it 1 paper
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To solve this problem, we now redo our analysis considering the warped compactification [ref] similar to the analysis of [ref] for the case of cold inflation.
Warm tachyonic inflation in warped background · Warm Inflation in Warped background · 0.83
Cites it as background 6 papers
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In particular, the 10D metric takes the form wcyds^2 = e^2Aη_μνdx^μdx^ν+e^-2A ds^2 for CY metric $ds^2$ and warp factor $A$ that depends on the internal space.[For convenience, $μ$ indices are denoted as raised with the Minkowski metric and warp factors are counted explicitly.] These compactifications develop “throat” regions where the warp factor becomes small and which can act as approximate Randall-Sundrum two-brane compactifications [ref] .
Warped Kaluza-Klein Dark Matter · Review of compactification and warped throat · 0.84
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It was famously realized in the Randall–Sundrum II [ref] and Karch–Randall models [ref] , for Minkowski and AdS spacetimes respectively, with string theory realizations explored for example in [ref] .
Can you hear the Planck mass? · Possible application to gravity localization · 0.96
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Localization can happen on a brane such as in [ref] or on a broader internal region, loosely referred to as “thick brane”.
Harmonic functions and gravity localization · Gravity localization in string theory · 0.94
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