Isotropic cosmological model with aetherically active axionic dark matter

In the framework of the extended Einstein-aether-axion theory we study the model of a two-level aetheric control over the evolution of a spatially isotropic homogeneous Universe filled with axionic dark matter. Two guiding functions are introduced, which depend on the expansion scalar of the aether...

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Bibliographic Details
Published in:arXiv.org 2024-01
Main Authors: Balakin, Alexander B, Shakirzyanov, Amir F
Format: Article
Language:English
Subjects:
Astronomical models
Cosmological constant
Cosmology
Dark matter
Exact solutions
Hypothetical particles
Online Access:Get full text
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Summary:In the framework of the extended Einstein-aether-axion theory we study the model of a two-level aetheric control over the evolution of a spatially isotropic homogeneous Universe filled with axionic dark matter. Two guiding functions are introduced, which depend on the expansion scalar of the aether flow, equal to the tripled Hubble function. The guiding function of the first type enters the aetheric effective metric, which modifies the kinetic term of the axionic system; the guiding function of the second type predetermines the structure of the potential of the axion field. We obtained new exact solutions of the total set of master equations of the model (with and without cosmological constant), and studied in detail four analytically solvable submodels, for which both guiding functions are reconstructed and illustrations of their behavior are presented.
ISSN:2331-8422
DOI:10.48550/arxiv.2401.16460