Abstract
We study a two-parameter family of exactly solvable inflation models with variable sound speed, and derive a corresponding exact expression for the spectrum of curvature perturbations. We generalize this expression to the slow-roll case, and derive an approximate expression for the scalar spectral index valid to second order in slow roll. We apply the result to the case of Dirac-Born-Infeld inflation, and show that for certain choices of slow-roll parameters, the Bunch-Davies limit (a) does not exist, or (b) is sensitive to stringy physics in the bulk, which in principle can have observable signatures in the primordial power spectrum.
| Original language | English |
|---|---|
| Article number | 103517 |
| Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 77 |
| Issue number | 10 |
| DOIs | |
| State | Published - May 21 2008 |
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