Anisotropic fractional cosmology: K-essence theory
J. Socorro, J. Juan Rosales, L. Toledo Sesma

TL;DR
This paper explores fractional differential equations arising in anisotropic K-essence cosmology within quantum and classical frameworks, providing exact solutions and analyzing the impact of fractional calculus on cosmological models.
Contribution
It introduces fractional differential equations in the Wheeler-DeWitt equation for anisotropic K-essence cosmology and derives exact classical and quantum solutions, highlighting the role of fractional calculus.
Findings
Fractional differential equations depend on the barotropic parameter.
Exact classical solutions are obtained in different gauges.
Quantum solutions are derived using fractional power series.
Abstract
In the particular configuration of the scalar field K-essence in the Wheeler-DeWitt quantum equation, for some age in the Bianchi type I anisotropic cosmological model, a fractional differential equation for the scalar field arises naturally. The order of the fractional differential equation is . This fractional equation belongs to different intervals, depending on the value of the barotropic parameter; when , the order belongs to the interval , and when , the order belongs to the interval . In the quantum scheme, we introduce the factor ordering problem in the variables and its corresponding momenta , obtaining a linear fractional differential equation with variable coefficients in the scalar field equation, then the solution is…
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Taxonomy
TopicsCosmology and Gravitation Theories
