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Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation

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arxiv astro-ph/0505158 v3 pith:55R4SM7B submitted 2005-05-09 astro-ph hep-ph

classification astro-phhep-ph
keywords analysisapproximationgeneralmodesslow-rolldatainflatonobservables
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abstract

Through a principal component analysis, we study how accurately CMB observables can constrain inflaton potentials in a model independent manner. We apply the general slow-roll approximation in our analysis where we allow, in contrast to the standard slow-roll approximation, the possibility of variations in $V''(\phi)$ and take into account the fact that horizon crossing is not an instantaneous event. Our analysis provides a set of modes to be used in fitting observables. We find that of order five of these modes will be constrained by future observations, so a fully general data analysis package could use the amplitudes of just a handful of modes as free parameters and retain all relevant information in the data.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Inverse-Scattering Reconstruction of Inflation from Scalar and Tensor Primordial Spectra

    astro-ph.CO 2026-06 unverdicted novelty 7.0 of 10

    An inverse-scattering method reconstructs inflationary potentials from primordial power spectra using Jost functions derived from the Mukhanov-Sasaki equation.

  2. Raising the reionization optical depth with inflationary CMB features

    astro-ph.CO 2026-06 unverdicted novelty 4.0 of 10

    Marginalizing over generalized slow-roll inflationary templates for the CMB low-power feature raises the 95% upper limit on τ to 0.075 (Planck) or 0.082 (all CMB+BAO), resolving incompatibility with lower bounds.

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