On 3+1 Dimensional Friedman-Robertson-Walker Universes with Matter
T. Christodoulakis, C. Helias, P.G. Kevrekidis, I.G. Kevrekidis and, G.O. Papadopoulos

TL;DR
This paper investigates the behavior of matter fields in 3+1 dimensional Friedmann-Robertson-Walker universes, revealing nonlinear dynamics and finite-time blowup phenomena with implications for quantum cosmology.
Contribution
It provides new analytical solutions for scalar fields coupled to gravity in cosmological models, highlighting nonlinear effects and potential links to quantum cosmology.
Findings
Regular solutions in the massless case
Asymptotic solutions in the massive case
Finite-time blowup phenomena
Abstract
We examine the dynamical behavior of matter coupled to gravity in the context of a linear Klein-Gordon equation coupled to a Friedman-Robertson-Walker metric. The resulting ordinary differential equations can be decoupled, the effect of gravity being traced in rendering the equation for the scalar field nonlinear. We obtain regular (in the massless case) and asymptotic (in the massive case) solutions for the resulting matter field and discuss their ensuing finite time blowup in the light of earlier findings. Finally, some potentially interesting connections of these blowups with features of focusing in the theory of nonlinear partial differential equations are outlined, suggesting the potential relevance of a nonlinear theory of quantum cosmology.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
