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  4. Phenomenology of D-Brane Inflation with General Speed of Sound
 
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Phenomenology of D-Brane Inflation with General Speed of Sound

Journal
Phys.Rev.D76:103517,2007
Journal Volume
76
Journal Issue
10
Date Issued
2007-06-09
Author(s)
Hiranya V. Peiris
Daniel Baumann  
Brett Friedman
Asantha Cooray
DOI
10.1103/PhysRevD.76.103517
URI
https://scholars.lib.ntu.edu.tw/handle/123456789/639957
URL
http://arxiv.org/abs/0706.1240v3
Abstract
A characteristic of D-brane inflation is that fluctuations in the inflaton field can propagate at a speed significantly less than the speed of light. This yields observable effects that are distinct from those of single-field slow roll inflation, such as a modification of the inflationary consistency relation and a potentially large level of non-Gaussianities. We present a numerical algorithm that extends the inflationary flow formalism to models with general speed of sound. For an ensemble of D-brane inflation models parameterized by the Hubble parameter and the speed of sound as polynomial functions of the inflaton field, we give qualitative predictions for the key inflationary observables. We discuss various consistency relations for D-brane inflation, and compare the qualitative shapes of the warp factors we derive from the numerical models with analytical warp factors considered in the literature. Finally, we derive and apply a generalized microphysical bound on the inflaton field variation during brane inflation. While a large number of models are consistent with current cosmological constraints, almost all of these models violate the compactification constraint on the field range in four-dimensional Planck units. If the field range bound is to hold, then models with a detectable level of non-Gaussianity predict a blue scalar spectral index, and a tensor component that is far below the detection limit of any future experiment.
Subjects
Astrophysics; Astrophysics; High Energy Physics - Theory
SDGs

[SDGs]SDG8

Description
23 pages, 11 figures, v2: version accepted by PRD; minor
clarifications and references added to the text. Higher resolution figures
are available in the published version. v3: post-publication correction of
typo in Eq. 87. No results/conclusions changed
Type
journal article

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