arXiv · 2101.03981
$\alpha$-Attractors and Reheating in a Non-Minimal Inflationary Model
Abstract
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.
Explore related subjects
Keep this discovery
Raheleh Shojaee, Kourosh Nozari, Farhad Darabi. 2021-01-11. $\alpha$-Attractors and Reheating in a Non-Minimal Inflationary Model. https://doi.org/10.1142/s0218271820500777
Cite the original work for its findings. Save a collection to share your selection of sources.