An Inflationary Model with an Exact Perturbation Spectrum
arXiv:astro-ph/9511143 · doi:10.1088/0264-9381/13/7/011
Abstract
We present a new, exact scalar field cosmology for which the spectrum of scalar (density) perturbations can be calculated exactly. We use this exact result to the probe the accuracy of approximate calculations of the perturbation spectrum.
7 pages, plus 2 figures
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