English

DBI N-flation

High Energy Physics - Theory 2009-05-20 v3 Astrophysics

Abstract

We investigate DBI inflation using NN multiple branes and show how the configuration is equivalent to a single wrapped D5D5-brane with flux. We then show how 1/N corrections can be implemented, and we examine the sound speed and levels of non-Gaussianities in two distinct cases. For models with constant warping we find that the non-Gaussian amplitude is bounded from above (as a function of γ\gamma). For AdSAdS backgrounds we find that the signature is generally large and positive, although is no longer globally defined over the full phase space. We then investigate an inflationary mechanism using a representation cascade, whereby the transition from a reducible representation to the irrep drives inflation.

Keywords

Cite

@article{arxiv.0711.0760,
  title  = {DBI N-flation},
  author = {John Ward},
  journal= {arXiv preprint arXiv:0711.0760},
  year   = {2009}
}

Comments

33 pages, 8 figures. References added and typos corrected. Submitted to JHEP

R2 v1 2026-06-21T09:40:06.971Z