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• W2022032011 abstract "Through a principal component analysis, we study how accurately cosmic microwave background 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 ${V}^{ensuremath{'}ensuremath{'}}(ensuremath{phi})$ 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." @default.
• W2022032011 created "2016-06-24" @default.
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• W2022032011 date "2005-07-12" @default.
• W2022032011 modified "2023-09-24" @default.
• W2022032011 title "Precision of inflaton potential reconstruction from CMB using the general slow-roll approximation" @default.
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• W2022032011 doi "https://doi.org/10.1103/physrevd.72.023510" @default.
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