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Code for computing the mode evolution of inflaton and curvature perturbations in single field inflation models.

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RM503/PBH_from_USR_inflation

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Inflation_Mukhanov_Sasaki_solver

Code for solving inflaton background dynamics for the computation of the mode evolution in inflationary models. The differential equations (both background and perturbation) are solved using a fourth-order Runge-Kutta (RK4) method.

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Code for computing the mode evolution of inflaton and curvature perturbations in single field inflation models.

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