Dynamical Properties of the Mukhanov-Sasaki Hamiltonian in the Context of Adiabatic Vacua and the Lewis-Riesenfeld Invariant

We use the method of the Lewis-Riesenfeld invariant to analyze the dynamical properties of the Mukhanov-Sasaki Hamiltonian and, following this approach, investigate whether we can obtain possible candidates for initial states in the context of inflation considering a quasi-de Sitter spacetime. Our m...

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Bibliographic Details
Main Authors: Max Joseph Fahn, Kristina Giesel, Michael Kobler
Format: Article
Language:English
Published: MDPI AG 2019-07-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/5/7/170