Kumar, K. SravanMarto, JoãoMoniz, PauloDas, Suratna2018-11-262018-11-262015-12-28http://hdl.handle.net/10400.6/6506We study inflation in the alpha-attractor model under a non-slow-roll dynamics with an ansatz proposed by Gong & Sasaki of assuming N=N(phi). Under this approach, we construct a class of local shapes of inflaton potential that are different from the T-models. We find this type of inflationary scenario predicts an attractor at n_s~0.967 and r~0.00055. In our approach, the non-slow-roll inflaton dynamics are related to the $\alpha-$parameter which is the curvature of Kähler geometry in the SUGRA embedding of this model.engInflationSupergravityGravitational waves in α-attractorsbook part10.1142/9789813226609_0571