Higher-order modified Starobinsky inflation
arXiv:1810.08911 · doi:10.1088/1475-7516/2019/02/055
Abstract
An extension of the Starobinsky model is proposed. Besides the usual Starobinsky Lagrangian, a term proportional to the derivative of the scalar curvature, , is considered. The analyzis is done in the Einstein frame with the introduction of a scalar field and a vector field. We show that inflation is attainable in our model, allowing for a graceful exit. We also build the cosmological perturbations and obtain the leading-order curvature power spectrum, scalar and tensor tilts and tensor-to-scalar ratio. The tensor and curvature power spectrums are compared to the most recent observations from BICEP2/Keck collaboration. We verify that the scalar-to-tensor rate can be expected to be up to three times the values predicted by Starobinsky model.
32 pages, 10 figures, minor changes, new references added
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