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Towards multi-field D-brane inflation in a warped throat
High Energy Physics - Theory · Submitted 13 Jul 2010
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Inflation is realized by the motion of a D-brane along the radial direction of the throat, and at later stages instabilities develop in the angular directions.
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The abstract, sentence by sentence
We study the inflationary dynamics in a model of slow-roll inflation in warped throat. Inflation is realized by the motion of a D-brane along the radial direction of the throat, and at later stages instabilities develop in the angular directions. We closely investigate both the single field potential relevant for the slow-roll phase, and the full multi-field one including the angular modes which becomes important at later stages. We study the main features of the instability process, discussing its possible consequences and identifying the vacua towards which the angular modes are driven.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We study the inflationary dynamics in a model of slow-roll inflation in warped throat. | contribution 0.95 | 0.90 | 0.04 | asserted 0.93 |
| s1 | Inflation is realized by the motion of a D-brane along the radial direction of the throat, and at later stages instabilities develop in the angular directions. | method 0.47 | 0.56 | 0.18 | asserted 1.00 |
| s2 | We closely investigate both the single field potential relevant for the slow-roll phase, and the full multi-field one including the angular modes which becomes important at later stages. | contribution 0.89 | 0.94 | 0.08 | asserted 0.94 |
| s3 | We study the main features of the instability process, discussing its possible consequences and identifying the vacua towards which the angular modes are driven. | contribution 0.89 | 0.94 | 0.28 | asserted 0.75 |
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The paper
Original abstract
We study the inflationary dynamics in a model of slow-roll inflation in warped throat. Inflation is realized by the motion of a D-brane along the radial direction of the throat, and at later stages instabilities develop in the angular directions. We closely investigate both the single field potential relevant for the slow-roll phase, and the full multi-field one including the angular modes which becomes important at later stages. We study the main features of the instability process, discussing its possible consequences and identifying the vacua towards which the angular modes are driven.
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References
How the literature uses it
9 arXiv papers cite this in 20 sentences
Papers citing it · 18 sentences without a confident label
Cites it as background 2 papers
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In recent years there has been significant progress within the `KKLT' framework, [ref] , in which the older idea of brane inflation [ref] , is realised via the motion of a brane in internal, hidden, extra dimensions [ref] (see also [ref] and the reviews [ref] ).
Spinflation with Angular Potentials · Introduction · 1.00
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Multifield inflationary models open up even further possibilities, such as curvatons [ref] , turning [ref] or bifurcating [ref] trajectories, thermal effects [ref] and etc [For a recent review on non-Gaussian effects for different inflationary models, see [ref] which also contains an organized classification of different types of non-Gaussianity.].
A Note on Calm Excited States of Inflation · Introduction · 0.89
What it cites · 61 sentences without a confident label
Uses the method or tool of 3 papers
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To study the D3 trajectory in such a throat, an elegant systematic way to parametrize the potential experienced by a D3-brane was recently given in Refs. [ref] , which can be summarized succintly as
Holographic Systematics of D-brane Inflation · Parametrizing the potential and multiple field inflation · 0.94
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To study the D3 trajectory in such a throat, an elegant systematic way to parametrize the potential experienced by a D3-brane was recently given in Refs. [ref] , which can be summarized succintly as
D3-brane Potentials from Fluxes in AdS/CFT · Parametrizing the potential and multiple field inflation · 0.94
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To parametrize the angular coordinate $Ψ_i$, we can rewrite the matrix $W$ as [ref]
Towards an Explicit Model of D-brane Inflation · Extremal trajectory and angular mass matrix · 0.87
Compares with 1 paper
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The observational predictions from slow-roll inflation is very similar to those in the Kuperstein embedding [ref] .
Towards a warped inflationary brane scanning · Slow-roll inflation in the Ouyang embedding · 1.00
Cites as support 3 papers
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Notice that, as shown in Ref. [ref] , if the separation between brane and antibrane is sufficiently large, the Coulomb potential does not depend on the angular coordinates.
Towards Inflation in String Theory · An explicit inflaton potential: Ouyang embedding case · 0.96
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As shown in Ref. [ref] , the main point to notice is that bulk contributions to the angular potential give rise to suppressed by powers of the warp factor.
D3-brane Vacua in Stabilized Compactifications · Slow-roll inflation in the Ouyang embedding · 0.97
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As shown in Ref. [ref] , this force is generically suppressed with respect to the other contributions to the D3 potential.
Towards an Explicit Model of D-brane Inflation · An explicit inflaton potential: Ouyang embedding case · 0.99
Cites as background 15 papers
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The parametric solution to ([ref]) have been extensively investigated in Refs. [ref] .
Holographic Systematics of D-brane Inflation · Parametrizing the potential and multiple field inflation · 0.89
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The parametric solution to ([ref]) have been extensively investigated in Refs. [ref] .
D3-brane Potentials from Fluxes in AdS/CFT · Parametrizing the potential and multiple field inflation · 0.89
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In the original model, a Kuperstein-embedded D7-brane on the warped conifold [ref] was considered, and the non-perturbative gaugino condensation on its worldvolume contributes to stabilize all the moduli besides the inflaton.
Meson spectroscopy from holomorphic probes on the warped deformed conifold · Introduction and summary · 0.81
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