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arXiv:2101.03981 [astro-ph.CO]AbstractReferencesReviewsResources

α-Attractors and Reheating in a Non-Minimal Inflationary Model

Raheleh Shojaee, Kourosh Nozari, Farhad Darabi

Published 2021-01-11Version 1

We study {\alpha}-attractor models with both E-model and T-model potential in an extended Non-Minimal Derivative (NMD) inflation where a canonical scalar field and its derivatives are non-minimally coupled to gravity. We calculate the evolution of perturbations during this regime. Then by adopting inflation potentials of the model we show that in the large N and small {\alpha} limit, value of the scalar spectral index ns and tensor to scalar ratio r are universal. Next, we study reheating after inflation in this formalism. We obtain some constraints on the model's parameter space by adopting the results with Planck 2018.

Comments: 17 pages, 7 figures
Journal: Int. J. Mod. Phys. D, Vol. 29, No. 10, 2050077 (2020)
Categories: astro-ph.CO, gr-qc, hep-th
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