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- W3204373909 abstract "We discuss the impact of the preheating stage due to the interaction of the inflaton to fermions in Palatini formulation. In Palatini inflation with large non-minimal coupling, the field is allowed to return to the plateau region during the reheating stage, therefore the average equation of state per oscillations is closer to -1 rather than 1/3. The incursion in the plateau, however, leads to a highly efficient tachyonic instability, which is able to reheat the Universe in less than one e-fold. By taking prescription II into account, which is discussed in the literature, we calculate the spectral index n_s and the tensor-to-scalar ratio r in the wide range of κ- ξ. We will show the results which are compatible with the data given by the Keck Array/BICEP2 and Planck collaborations." @default.
- W3204373909 created "2021-10-11" @default.
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- W3204373909 date "2021-09-24" @default.
- W3204373909 modified "2023-09-30" @default.
- W3204373909 title "Preheating in radiatively corrected φ4 inflation with non-minimal coupling in Palatini formulation" @default.
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- W3204373909 doi "https://doi.org/10.17776/csj.892438" @default.
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