From the Spectrum to Inflation: A Second Order Inverse Formula for the General Slow-Roll Spectrum
arXiv:astro-ph/0511476 · doi:10.1088/1475-7516/2006/02/005
Abstract
We invert the second order, single field, general slow-roll formula for the power spectrum, to obtain a second order formula for inflationary parameters in terms of the primordial power spectrum.
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Cited by in corpus (6)
- Inflationary Potential Reconstruction for a WMAP Running Power Spectrum
- Correlating correlation functions of primordial perturbations
- Can power spectrum observations rule out slow-roll inflation?
- Potential reconstruction from general power spectrum in single-field inflation
- Inflationary Hubble Parameter from the Gravitational Wave Spectrum in the General Slow-roll Approximation
- Mimicking two field inflationary features with a single field