Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations
arXiv:0710.1812 · doi:10.1103/PhysRevD.77.023527
Abstract
We compare the Infrared Dirac-Born-Infeld (IR DBI) brane inflation model to observations using a Bayesian analysis. The current data cannot distinguish it from the \LambdaCDM model, but is able to give interesting constraints on various microscopic parameters including the mass of the brane moduli potential, the fundamental string scale, the charge or warp factor of throats, and the number of the mobile branes. We quantify some distinctive testable predictions with stringy signatures, such as the large non-Gaussianity, and the large, but regional, running of the spectral index. These results illustrate how we may be able to probe aspects of string theory using cosmological observations.
54 pages, 13 figures. v2: non-Gaussianity constraint has been applied to the model; parameter constraints have tightened significantly, conclusions unchanged. References added; v3, minor revision, PRD version
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Cited by in corpus (24)
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- Holographic Systematics of D-brane Inflation
- Chasing Brane Inflation in String-Theory
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- Reconstructing a general inflationary action
- K-inflationary Power Spectra in the Uniform Approximation
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- Constraints on Kinetically Modified Inflation from WMAP5
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- Fine-Tuning in DBI Inflationary Mechanism
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- Reconstructing Single Field Inflationary Actions From CMBR Data
- Different approaches to the second order Klein-Gordon equation
- On the four-dimensional effective theories in brane-worlds
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