Precision Predictions for the Primordial Power Spectra from f(R) Models of Inflation
arXiv:1606.05879 · doi:10.1016/j.nuclphysb.2016.08.010
Abstract
We study the power spectra of f(R) inflation using a new technique in which the norm-squared of the mode functions is evolved. Our technique results in excellent analytic approximations for how the spectra depend upon the function . Although the spectra are numerically the same in the Jordan and Einstein frames for the same wave number , they depend upon the geometries of these frames in quite different ways. For example, the power spectra in the two frames are different functions of the number of e-foldings until end of inflation. We discuss how future data on reheating can be used to distinguish f(R) inflation from scalar-driven inflation.
arXiv comment27 pages, 8 figures, uses LaTeX2e Version 2 slightly revised for publication
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