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Initial conditions in chaotic inflation with modified gravity

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Figure

Figure 1. In a model of chaotic inflation with largefield [1] the inflaton slowly rolls along the potentialslope mimicking almost constant energy density, sothe Universe exhibits (almost) exponential expansion.The slow rolling stops at some point and the infla
Figure 2. Cosmological constraints [4] on inflationary models. The colored regions are allowed at 95% CL, thereare predictions of various cosmological models.
Figure 3. Examples of a flat potential in R2-inflation (left panel) and Higgs-inflation (right panel).

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