Interaction of the Cosmic Dark Fluid with Dynamic Aether: Parametric Mechanism of Axion Generation in the Early Universe
Alexander B. Balakin, Alexei S. Ilin, Amir F. Shakirzyanov

TL;DR
This paper presents a cosmological model with five interacting components, demonstrating how dynamic aether and rheologic dark fluid influence early universe evolution and enable a parametric mechanism for axion generation.
Contribution
It introduces a novel five-element cosmological model incorporating dynamic aether and rheologic dark energy, revealing new epochs and axion growth mechanisms.
Findings
Early universe exhibits super-inflation and oscillatory epochs.
Oscillations induce a Floquet-type parametric axion growth.
Dynamic aether regulates spacetime evolution.
Abstract
We consider an isotropic homogeneous cosmological model with five interacting elements: first, the dynamic aether presented by a unit timelike vector field, second, the pseudoscalar field describing an axionic component of the dark matter, third, the cosmic dark energy, described by a rheologic fluid, fourth, the non-axionic dark matter coupled to the dark energy, fifth, the gravity field. We show that the early evolution of the Universe described by this model can include two specific epochs: the first one can be characterized as a super-inflation, the second epoch is associated with an oscillatory regime. The dynamic aether carries out a regulatory mission; the rheologic dark fluid provides the specific features of the spacetime evolution. The oscillations of the scale factor and of the Hubble function are shown to switch on the parametric (Floquet - type) mechanism of the axion…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
