Turbulence-Stabilized Axionic Solitons in Galactic Environments

This working paper introduces the TSAS (Turbulence-Stabilized Axionic Solitons) hypothesis, proposing that axionic solitons can be dynamically stabilized through interactions with quantum turbulence in galactic environments. The hypothesis derives a dual scaling law linking the de Broglie wavelength to turbulent dissipation scales, rooted in Kolmogorov-like cascades adapted for axion fluid dynamics. Entropy evolution, Feynman vertex interactions, pulsar timing predictions, and cosmological abundance models are incorporated to support testability. The framework aligns with upcoming observational capabilities (SKA, JWST, PTA) and includes falsifiable predictions across multiple domains, from neutron star interiors to CMB constraints. The author developed this hypothesis using theoretical modeling, thermodynamic formalism, and symbolic computation with assistance from AI tools for verification, formatting, and research. This document is intended as an open scientific contribution from a secondary school student in Kazakhstan and is archived under DOI: 10.5281/zenodo.15751668.