Algebraic integrability of FRW-scalar cosmologies
Spiros Cotsakis, John Miritzis

TL;DR
This paper investigates the integrability of isotropic cosmological models in general relativity and string theory using Painlevé analysis to determine the presence of solutions with the necessary arbitrary constants.
Contribution
It applies Painlevé analysis to assess the algebraic integrability of FRW-scalar cosmologies, extending the understanding of chaos and solvability in these models.
Findings
Determines conditions for integrability in various cosmological models
Identifies cases where solutions admit Laurent expansions with arbitrary constants
Provides criteria for chaos versus integrability in cosmological dynamics
Abstract
For dynamical systems of dimension three or more the question of integrability or nonintegrability is extended by the possibility of chaotic behaviour in the general solution. We determine the integrability of isotropic cosmological models in general relativity and string theory with a variety of matter terms, by a performance of the Painlev\'{e} analysis in an effort to examine whether or not there exists a Laurent expansion of the solution about a movable pole which contains the number of arbitrary constants necessary for a general solution.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Particle physics theoretical and experimental studies
