arXiv · hep-ph/9304228
Observing the Inflaton Potential
Abstract
We show how observations of the density perturbation (scalar) spectrum and the gravitational wave (tensor) spectrum allow a reconstruction of the potential responsible for cosmological inflation. A complete functional reconstruction or a perturbative approximation about a single scale are possible; the suitability of each approach depends on the data available. Consistency equations between the scalar and tensor spectra are derived, which provide a powerful signal of inflation.
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Edmund J. Copeland, Edward W. Kolb, Andrew R. Liddle, James E. Lidsey. 1993-04-07. Observing the Inflaton Potential. https://doi.org/10.1103/physrevlett.71.219
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