Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric

We study the quantum cosmology of a quadratic fR theory with a FRW metric, via one of its equivalent Horndeski type actions, where the dynamic of the scalar field is induced. The classical equations of motion and the Wheeler-DeWitt equation, in their exact versions, are solved numerically. There is...

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Main Authors: V. Vázquez-Báez, C. Ramírez
Format: Article
Language:English
Published: Wiley 2017-01-01
Series:Advances in Mathematical Physics
Online Access:http://dx.doi.org/10.1155/2017/1056514
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author V. Vázquez-Báez
C. Ramírez
author_facet V. Vázquez-Báez
C. Ramírez
author_sort V. Vázquez-Báez
collection DOAJ
description We study the quantum cosmology of a quadratic fR theory with a FRW metric, via one of its equivalent Horndeski type actions, where the dynamic of the scalar field is induced. The classical equations of motion and the Wheeler-DeWitt equation, in their exact versions, are solved numerically. There is a free parameter in the action from which two cases follow: inflation + exit and inflation alone. The numerical solution of the Wheeler-DeWitt equation depends strongly on the boundary conditions, which can be chosen so that the resulting wave function of the universe is normalizable and consistent with Hermitian operators.
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spelling doaj-art-46e28956e7a648b083da067d03582c252025-02-03T01:32:22ZengWileyAdvances in Mathematical Physics1687-91201687-91392017-01-01201710.1155/2017/10565141056514Quantum Cosmology of Quadratic f(R) Theories with a FRW MetricV. Vázquez-Báez0C. Ramírez1Facultad de Ingeniería, Benemérita Universidad Autónoma de Puebla, 72000 Puebla, PUE, MexicoFacultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, P.O. Box 165, 72000 Puebla, PUE, MexicoWe study the quantum cosmology of a quadratic fR theory with a FRW metric, via one of its equivalent Horndeski type actions, where the dynamic of the scalar field is induced. The classical equations of motion and the Wheeler-DeWitt equation, in their exact versions, are solved numerically. There is a free parameter in the action from which two cases follow: inflation + exit and inflation alone. The numerical solution of the Wheeler-DeWitt equation depends strongly on the boundary conditions, which can be chosen so that the resulting wave function of the universe is normalizable and consistent with Hermitian operators.http://dx.doi.org/10.1155/2017/1056514
spellingShingle V. Vázquez-Báez
C. Ramírez
Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric
Advances in Mathematical Physics
title Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric
title_full Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric
title_fullStr Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric
title_full_unstemmed Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric
title_short Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric
title_sort quantum cosmology of quadratic f r theories with a frw metric
url http://dx.doi.org/10.1155/2017/1056514
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