On the power spectrum of inflationary cosmologies dual to a deformed CFT
arXiv:1308.0331 · doi:10.1007/JHEP10(2013)071
Abstract
We analyse slow-roll inflationary cosmologies that are holographically dual to a three-dimensional conformal field theory deformed by a nearly marginal scalar operator. We show the cosmological power spectrum is inversely proportional to the spectral density associated with the 2-point function of the trace of the stress tensor in the deformed CFT. Computing this quantity using second-order conformal perturbation theory, we obtain a holographic power spectrum in exact agreement with the expected inflationary power spectrum to second order in slow roll.
26 pp, 4 figs
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