Building analytical three-field cosmological models

Abstract

A difficult task to deal with is the analytical treatment of models composed by three real scalar fields, once their equations of motion are in general coupled and hard to be integrated. In order to overcome this problem we introduce a methodology to construct three-field models based on the so-called "extension method". The fundamental idea of the procedure is to combine three one-field systems in a non-trivial way, to construct an effective three scalar field model. An interesting scenario where the method can be implemented is within inflationary models, where the Einstein-Hilbert Lagrangian is coupled with the scalar field Lagrangian. We exemplify how a new model constructed from our method can lead to non-trivial behaviors for cosmological parameters.

arXiv comment11 pages, and 3 figures, updated version published in EPJC

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Cited by in corpus (4)

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• Extended multi-scalar field theories in (1+1) dimensions
• Localized structures in three-field models: geometrically constrained configurations and the first-order framework
• New family of potentials with analytical twiston-like solutions