Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations
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.
Keywords
Cite
@article{arxiv.0710.1812,
title = {Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations},
author = {Rachel Bean and Xingang Chen and Hiranya V. Peiris and Jiajun Xu},
journal= {arXiv preprint arXiv:0710.1812},
year = {2008}
}
Comments
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